Contents of: II/250/./gcvs_rem.dat

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## (from tabmap V6.0 (2016-08-18)) 2024-03-29T15:07:44
#---------------------------------------------------------------------------
#-- II/250 Combined General Catalogue of Variable Stars (Samus+ 2004)
#--------------------------------------------------------------------------
#---Table: II/250/./gcvs_rem.dat Remarks on GCVS stars  (14441 records)
#      GCVS A10    ---   Variable star designation
#      Text A81    ---   Text of note.
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GCVS      |Text
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R     And |S5/4.5e.
S     And |SN (NGC 224).
W     And |S7.5/1-e.
X     And |S5/7-e.
Z     And |The light curve is characterized
Z     And |by outbursts up to 4m with intervals of 10 - 20
Z     And |years. In the intervals cyclic variations are observed with
Z     And |the mean period of 632d and variations with cycles of
Z     And |several days and Delta(m) ~ 0.1m - 0.5m. The spectrum is
Z     And |symbiotic, with features of a late M giant, narrow
Z     And |low-excitation emission lines (Bleq) and forbidden lines
Z     And |characteristic of highly excited nebulae.
RR    And |S6/3.5e.
RT    And |Min II 8.88; DI = DII = 0.17P; dI = dII = 0.00. P var.
RT    And |Nonlinear term: -6.33*10**(-11)*E**2. During
RT    And |JD2433477 - 43878 linear elements are satisfactory:
RT    And |Min = 2441141.8888 + 0.62892984d*E. Period changes
RT    And |according to a sine law are possible [08002].
RU    And |P var. Max = 2419857 + 243.0d*E (JD2412800 -
RU    And |20000); Max = 2434551 + 233.24d*E (JD2420000 -
RU    And |34550). Since JD2435000 - see Table. Delta(m) ~ 4m - 5m
RU    And |(before JD2429600), ~1m (JD2429600 ~ 33600), up to 3m
RU    And |(JD ~2436000),  ~1.5m (JD ~2436700). In 1970 - 1972
RU    And |showed quite irregular variations.
RX    And |SB (P = 0.21173d). Cyclic variations with P ~ 38s - 54s
RX    And |were observed after a normal maximum; after a short
RX    And |maximum no periodicity was found [08004].
SS    And |Two long period variations are also observed:
SS    And |P = 650d, P = 3800d.
ST    And |P var. Max = 2418370 + 337.3d*E (JD2418000 - 28000).
ST    And |Since JD2428000 - see Table.
SU    And |VB A (B 12.77m V, F0V:, 15").
SV    And |The magnitude in Max varies periodically, P = 930d,
SV    And |P = 5400d? [02146].
SW    And |[Fe/H] = +0.16. P var. Nonlinear term:
SW    And |-1.229d*10**(-10)*E**2 [01959]. Since 1959
SW    And |Max = 2436466.828 + 0.442270121d*E [06929].
SW    And |The shape of the light curve varies with
SW    And |Pi ~36.83d = 83.28 P. The deviations (O - C) satisfy
SW    And |the elements of Blazhko effect
SW    And |Max(O - C) = 2436816.23 + 36.921d*N. Secular trend
SW    And |and cyclic (P ~2a) variations of (O - C) are possible
SW    And |[08005].
SY    And |d = 0.027P.
TT    And |Min II 11.6?
TU    And |P var (Pi ~37a?).
TV    And |P var? Delta(m) strongly varies.
TW    And |d = 0.020P. Min II 8.94. P var. Min = 2428845.422 +
TW    And |4.122739d*E (JD2420050 - 32000). Since JD2432000 - see
TW    And |Table.
TZ    And |P1 = 118d: [00882].
TZ    And |Mean magnitude varies with P2 = 974d [00098]. P = 135d
TZ    And |(JD2437545 - 38377) [03367].
UU    And |P var. Min = 2428832.536 + 1.486311d*E (JD2421455 - 23740)
UU    And |[02262]; Min = 2428832.465 + 1.48629d*E (JD2428830 - 35012)
UU    And |[00745]. Since JD2441100 - see Table.
UW    And |P var. Before JD2430000 Max = 2418585 + 236.7d*E. Since
UW    And |JD2436000 - see Table.
WW    And |d = 0.012P.
WX    And |P var. Max = 2422613.614 + 3.0012544d*E (JD2422610 - 34712)
WX    And |[01240]. The Table gives current elements. d = 0.03P
WX    And |in 1972 and probably varies.
WZ    And |Min II 11.9. P var [02262]. Min = 2435075.342 + 0.695662d*E
WZ    And |(before JD2440500); probably
WZ    And |Min = 2440872.290 + 0.6956576d*E since JD2440500.
WZ    And |The elements in the Table represent all the observations
WZ    And |satisfactorily.
XX    And |P var. Max = 2418001.938 + 0.7227486d*E (1908 - 1932);
XX    And |Max = 2427106.403 + 0.7227591d*E (1932 - 1946) [02264].
XX    And |Since 1946 - see Table. Delta(S) = 9. Blazhko effect:
XX    And |Max = 2437578 + 36d*N [03111].
XY    And |Blazhko effect is possible.
XZ    And |Min II 10.16; DII = 0.26P. P var [02431,06932,08008,08593]
XZ    And |Min = 2432883.6046 + 1.3572708d*E (JD2431700 - 36150)
XZ    And |[01977]; Min = 2441954.340 + 1.357293d*E
XZ    And |(since JD2436200). The elements in the Table represent all
XZ    And |the observations satisfactorily.
AA    And |Min II 10.5.
AB    And |Min II 10.20. P var. Period increased suddenly in 1953
AB    And |( ~JD2434500); no period changes later [02509,05222].
AB    And |Elements since 1953 - see Table.
AC    And |Unusual multiperiodical variable. Second oscillation:
AC    And |Max = 2432467.373 + 0.71124243d*E; P3 = 0.421069d [08187],
AC    And |see also [08294,08295]. Delta(S) = -1:.
AD    And |Min II 11.6. Depth of minima in yellow light: 0.62m (Min I),
AD    And |0.58m (Min II) [03141]. Min II - Min I = 0.494P. P var.
AD    And |Min = 2428718.402 + 0.9861940d*E (JD2417460 - 29640)
AD    And |[01983]. Since JD2428700 - see Table.
AE    And |In the M31 galaxy. Strong UV continuum.
AE    And |Emissions: H, He I, Fe II, [Fe II].
AF    And |In the M31 galaxy. Strong UV continuum.
AF    And |Emissions: H, He I, Fe II, [Fe II].
AG    And |According to [08296], DSCT:, Min = 2442636.5868 + 0.0347d*E,
AG    And |A = 0.5m.
AM    And |VB A (B 0.25' S).
AN    And |Min II 6.09. The existence of the third body in
AN    And |the system is possible. Sp(Met) = F2 - F5.
AP    And |Min II 11.9. The period may be 2 times shorter.
AT    And |B - V: +0.42, +0.56. Delta(S) = 3. See [08299] for data
AT    And |on period variations and a detailed study.
BD    And |Min II 11.4.
BE    And |Average cycle: 137d [01993,02267]; 156.8d after JD2431700.
BL    And |Depth of Min II 0.24m: P var? Min I = 2429491.255 +
BL    And |0.7223779d*E (JD2415800 - 33900) [01995]. Since JD2433900 -
BL    And |see Table.
BX    And |ADS 1671 A (B 9.7m, 20", 59deg). Min II 9.15. Possible
BX    And |period change from 0.61011222d to 0.61011534d (~1952).
BX    And |On the period changes see also [08657].
BY    And |According to [08658], SRB:.
CC    And |Possibly in a binary with Porb = 10.469d. Delta(m) and the
CC    And |light curve shape vary with a period 5.23714d or 10.469d
CC    And |[08016]. According to [03120], 4 periods are present:
CC    And |P2 = 0.0632083d. First overtone was not found. Other
CC    And |periods are resonances.
CG    And |P var: 3.7430d (1950), 3.7394d (1963) [05224].
CG    And |Cyclic period changes are possible.
CG    And |According to [06941], short period oscillations (P = 2h 04m)
CG    And |are present. A number of observers do not find short-term
CG    And |variability.
CM    And |According to [00821], Max = 2428380 + 140d*E and Max =
CM    And |2430616 + 124d*E, and the star resembles UU Her.
CN    And |Min II 9.96.
CO    And |d = 0.06P:
CP    And |d = 0.01P? Depth of Min II 0.05m?
CU    And |d > 0.034P ([06943], according to visual observations.)
DI    And |DCEP? [03165].
DK    And |EW?
DL    And |In the field of the open cluster NGC 7686.
DR    And |P var. Before ~JD2437000 Max = 2436078.384 + 0.5630609d*E
DR    And |[02275]; then P changed abruptly. Delta(m) changes by ~0.3m,
DR    And |Max A1 = 2436078.8 + 69.486d*N1, Max A2 = 2437646.65 +
DR    And |69.719d*N2. Other possible cycles are 2000d (interaction
DR    And |of cycles N1 and N2) and ~30 years [08019].
DS    And |In the field of the open cluster NGC 752. Min II 10.7.
DZ    And |According to [04008], type RCB, spectrum R. According to
DZ    And |[06945], since 1961 is in Max light all the time. According
DZ    And |to [06946], the spectrum is not characteristic of RCB stars.
DZ    And |According to [08660], the star was bright near the moments
DZ    And |of Min light given in [04008].
EG    And |P = 40d or 80d [08020].
EG    And |Absorption spectrum with overlaying emissions of high
EG    And |excitation [04434,08598]. Strong variable magnetic field
EG    And |[04435]. Long period variations of light are observed.
EG    And |Radial velocities profiles and equivalent widths of lines
EG    And |vary with P = 470d [08596] (SB? [08597]). Possibly is
EG    And |analogous to HM Sge [08598].
EH    And |IR excess. The presence of a dust envelope is possible.
EO    And |Very red.
EP    And |Min II 12.5.
ET    And |Delta(B) = 0.035m, Delta(U) = 0.07m.
ET    And |The Table gives the epoch of Max light. Observations may
ET    And |be represented by the periods 0.723d and 1.61553d
ET    And |[08022,07946]. According to [08023], in June - December 1977
ET    And |Min = 2443337.4725 + 0.49925d*E, other periods are
ET    And |not satisfied by observations. According to [08599],
ET    And |Max(U) = 2439751.28 + 0.617135d*E (1967 - 1971).
ET    And |SB, Max(Vr) = JD2443718.0 + 48.304d*E [08301].
ET    And |Photometric periods could not be found in radial
ET    And |velocities.
EX    And |Possible Min II 13.0:, Min II - Min I = 0.55P.
EY    And |I - K = 5.38;
EY    And |the presence of a dust envelope is possible [06947].
FF    And |10.35m - 10.42m V outside flares;  M - m = 0.50P.
FF    And |Porb = 2.170304d [08024]. According to photometric
FF    And |observations, P = 2.14d (1971), P = 2.15d (1972),
FF    And |P = 2.19d (1973) [06948].
FG    And |According to [04156], EA; Min = 2436074.528 + 0.99772d*E.
FL    And |d = 0.02P.
FZ    And |mu = 1", p = 64deg.
GK    And |Min II 11.5.
GN    And |ADS 409 A (B 13.3m, 2", 6deg; C 11.6m, 141", 130deg).
GN    And |Different authors give spectral types F0 III, F2V, Am
GN    And |(probably based on different criteria).
GP    And |Delta(m) changes with P2 = 0.64d.
GP    And |A wave with P3 = 0.012161d is present. The mean
GP    And |magnitude and the shape of the light curve vary
GP    And |[08302].
GQ    And |ADS 246 B (A = GX And; B 37", 61deg). B - V = +1.80.
GQ    And |X-ray source.
GR    And |Min (magnet.field) = 2442288 + 525d*E.
GR    And |Magnetic field varies (-250 to -1030 Gauss). Period of
GR    And |changes of C1 is near 1.5 years [07893]. According to [06257],
GR    And |period of changes in u is near 1 year or longer.
GS    And |B - V = +1.7 in normal light.
GX    And |ADS 246 A (B = GQ And, 37", 61deg). Delta(U) = 0.55m. SB?
GX    And |(conflicting data).
GY    And |SB1 (P = 273.2d [07324], P = 272.99d [08303]).
GY    And |For spectral changes, variations of light and magnetic
GY    And |field it is possible that P = 23a [07004] or 20.60a [08303].
GY    And |[08022] gives P ~36.5d and Delta(V) ~0.049m. Periods 4.92a
GY    And |and 1.8d may exist [08303].
GZ    And |B - V: +0.77, +0.82. ADS 1693 A (B 11.13m, 8", 31deg).
GZ    And |Min II 11.58. P var?
GZ    And |The period is based only on Minima I [06830] and
GZ    And |was improved with account of recent data.
HH    And |Subdwarf? [06581]. mu = 1.82", p = 176deg.
HI    And |B - V = 1.8m outside flares.
HN    And |Max(U) = 2438327.8 + 69.433d*E [08022]. SB
HN    And |(P = 106.27d [07435]).
HQ    And |According to [08659], a probable cataclysmic binary;
HQ    And |similarity to AM Her and AN UMa is noted.
HR    And |d = 0.05P.
HT    And |B - V = +0.60. In the region of M 31.
HU    And |Min II 17.2. In the region of M 31.
HV    And |According to [08659], a probable cataclysmic binary;
HV    And |similarity to AM Her and AN UMa is noted.
HY    And |In the region of M 31.
HZ    And |In the region of M 31. P > 100d. Red.
IL    And |d = 0.02P.
IM    And |In the region of M 31.8.
IO    And |According to [08659], a probable cataclysmic binary;
IO    And |similarity to AM Her and AN UMa is noted.
IP    And |d = 0.02P:.
KK    And |The light curve has double-wave shape
KK    And |[07740]. Long period variations were found [07955].
KU    And |I - K = 4.63.
KU    And |SR type is possible. Surrounded with a dust envelope [08029].
KX    And |SB2 (P = 38.908d).
KZ    And |ADS 16557 B (A 7.0m; B 15", 254).
LM    And |Min II 12.7.
LN    And |Delta(B) = 0.025.
LO    And |Min II 11.82.
V0369 And |VB (0".1, 128 deg, 1986.9).
V0374 And |Not identical with BD+44 422.
alf   And |SB (P = 96.6960d). VB A (B 11.2m, 80").
alf   And |Epoch of Max U light is given.
alf   And |Hbeta index varies in the range of ~0.02m with P
alf   And |~3h [08030]. Rapid rotation.
zet   And |Depth of Min II 0.1m. SB.
zet   And |Unstable light curve. Most notable
zet   And |variations on the rising branch of Max II [08030].
zet   And |Many peculiarities in the spectrum.
lam   And |SB1 (P = 20.52d).
omi   And |v sin i = 300 km/s; VB(0.3"; possibly
omi   And |also 0.05" - according to speckle-interferometric data).
omi   And |Shell spectrum appeared and disappeared several
omi   And |times since 1890. Different authors attributed
omi   And |the star to EB type. According to [05955], The changes
omi   And |of light may be explained also by intrinsic
omi   And |variations of a single shell star. They are represented
omi   And |by elements: Min I = 2439470.628 + 1.0185d*E.
omi   And |According to [02572], Min I = 2436174.430 +
omi   And |1.5998398d*E. The periodogram analysis shows
omi   And |a stable peak at P ~0.84d [08032]. A possible shell
omi   And |event was observed late in 1975.
S     Ant |Min II 6.87. P var?
T     Ant |CWB? P var. [A/H] =  -0.0. P = 5.9098d (JD2428187 -
T     Ant |34688), P = 5.8976d (JD2434688 - 37660) [05387].
T     Ant |The Table gives mean elements which satisfy all
T     Ant |observations well enough.
V     Ant |OH, H2O maser.
Z     Ant |Mean brightness varies with P = 1143d.
SW    Ant |Min II 14.6.
UZ    Ant |P var?
WY    Ant |P var. P = 0.57430871d (JD2414000 - 22070); P =
WY    Ant |0.57431618d (JD2422070 - 25600); P = 0.57431216d
WY    Ant |(JD2425600 - 29000) [01113]. (k - b)2 = 0.00.
WZ    Ant |Min II 11.8.
XX    Ant |Min II 9.1.
XY    Ant |Depth of Min II 0.3m - 0.5m pg.
XZ    Ant |Min II 10.2.
Z     Aps |Possibly also an eclipsing binary.
RT    Aps |Strong variations of period and the shape of
RT    Aps |the light curve [06152].
TY    Aps |Delta(S) = 3.
YY    Aps |The period is probably long.
AF    Aps |Min II 13.9.
AN    Aps |Min II 12.8.
AP    Aps |Min II 15.5.
AS    Aps |Min II 13.8.
AV    Aps |Depth of Min II 0.05m.
CE    Aps |P = 209d or 261d.
CY    Aps |Min II 13.0.
EF    Aps |Min II 12.6.
FY    Aps |Deep Min II.
GK    Aps |Min II 13.9. RRC type is possible.
GO    Aps |Min II 14.8. RR type is possible.
GQ    Aps |Min II 14.8.
GU    Aps |Min II 14.5.
GX    Aps |RV type is not excluded. The epoch of Min is given.
GY    Aps |Min II 14.2.
HL    Aps |Min II 12.6.
HO    Aps |Min II 13.7.
HT    Aps |Min II 14.3.
HV    Aps |Epoch of Min is given.
HX    Aps |Min II 14.4.
II    Aps |Min II 11.6.
IL    Aps |Epoch of Min is given.
IO    Aps |Min II 12.4.
IR    Aps |Min II 13.8.
IU    Aps |Min II 14.6.
IY    Aps |Min II 12.9.
KN    Aps |d ~0.03P.
KR    Aps |Possibly a slow eclipsing variable.
KT    Aps |Min II 15.2.
KV    Aps |Min II 13.6.
KZ    Aps |Smooth light
KZ    Aps |changes with superimposed variations of eclipsing
KZ    Aps |nature, with minima on JD2436729 and 2436808.
LM    Aps |RV type is possible.
LN    Aps |Min II 13.3.
LO    Aps |Min II 11.5.
MY    Aps |L19-2. P0 = 192.75s, P1 = 113.77s.
del 1 Aps |In a wide pair (delta2 Aps, 100", common mu).
kap 1 Aps |SB? VB A (B 11.27m V, 27").
R     Aqr |Symbiotic spectrum. Emissions of H, SII, OIII, FeII, NeIII,
R     Aqr |OII. Variable radio source. SiO maser. The secondary may
R     Aqr |be an accreting white dwarf. The star is embedded in an
R     Aqr |expanding gaseous nebula several hundred years
R     Aqr |old. A cycle ~24a and longer-term variations are
R     Aqr |possible in the changes of radial velocities and period.
U     Aqr |Strong bands of 12C2, CN,
U     Aqr |lines of SrII, YII in the spectrum; hydrogen deficiency.
U     Aqr |A probable halo star (Vr ~100 km/s.).
Z     Aqr |1969 - 70: P = 100d +- [05973].
RY    Aqr |P var. Min = 2433872.352 + 1.966598d*E (before
RY    Aqr |JD2428000); Min = 2440824.410 + 1.966620d*E
RY    Aqr |(JD2428000 - 41000); Min = 2440824.410 +
RY    Aqr |1.966611d*E (JD2441000 - 43800). Since
RY    Aqr |JD2443800 P = 1.966554d?
RY    Aqr |The Table gives elements representing
RY    Aqr |observations after JD2428000 with the accuracy +-0.1d.
ST    Aqr |Min II 9.37. P var. Min = 2423640.271 + 0.78101367d*E
ST    Aqr |(JD2423500 - 26000) [02037]. Since JD2439700 - see Table.
SU    Aqr |ADS 16318 A (B 10.7m, 5", 144deg). Min II 10.5. P var?
SV    Aqr |Cycle 200 - 300d is possible.
SW    Aqr |P var. (k - b)2 = 0.01.
SX    Aqr |P var? Delta(S) = 9.
SZ    Aqr |Epoch of Min is given.
TT    Aqr |VB A (B 15m, 3", 135deg).
TZ    Aqr |Delta(S) = 5.
VY    Aqr |Second outburst: Max ~JD2437897
VY    Aqr |(1962),  ~9m pg [03129].
WX    Aqr |Blazhko effect is possible.
XZ    Aqr |P var. Before JD2437913 P = 2.059187d.
YZ    Aqr |B - V = 0.49 (in Min). (k - b)2 = 0.06.
YZ    Aqr |Small fluctuations of period are possible.
AE    Aqr |Unusual flare X-ray system with pulsar. Becomes bluer
AE    Aqr |in Max. In Min B - V = +0.92. Shows rapid irregular
AE    Aqr |variations, which differ it from UV stars and UG
AE    Aqr |system, though the spectra are somewhat similar.
AE    Aqr |Simultaneous photoelectric and spectroscopic observations
AE    Aqr |[03131] show the existence of two types of flares:
AE    Aqr |1) intensification of emission lines accompanied by
AE    Aqr |brightening in U and B; 2) intensification of continuum
AE    Aqr |leading to brightening in U, B and V ("white flare").
AE    Aqr |Detailed spectroscopic investigation [01971].
AE    Aqr |Porb = 0.41165794d + 1.12*10**(-10)*E, The epoch
AE    Aqr |T0 = JD2439030.621 [08672]. In the X-ray band
AE    Aqr |(0.1 - 4.0 keV) pulsations with P = 33.0767s are observed
AE    Aqr |[08673]. In the optical range pulsations with
AE    Aqr |P0 = 33.076737s as well as with P1 = 16.5s were noted
AE    Aqr |[08674,08675].
AT    Aqr |Min II 14.7.
AX    Aqr |P var. Before ~JD2427367 Max = 2425417.60 + 0.388135d*E
AX    Aqr |[03113].
AY    Aqr |Min II 14.3.
BH    Aqr |P var. Before ~JD2431150 Max = 2426948.411 + 0.5258022d*E
BH    Aqr |[03113].
BI    Aqr |Min II 13.1.
BK    Aqr |Close companion.
BL    Aqr |Waves from 80 to 125d. Mean magnitude changes
BL    Aqr |with cycles from 480 to 700d in the range of 0.3m - 0.6m.
BM    Aqr |The mean magnitude may vary with P = 500 - 600d.
BN    Aqr |Delta(S) = 4:. P var. Before JD2428964 Max =
BN    Aqr |2426577.901 + 0.46963401d*E [03113].
BN    Aqr |According to [05391] Max = 2429395.742 +
BN    Aqr |0.4696410d*E + 3.3*10**(-10)*E**2 (1898 - 1958).
BO    Aqr |P var? (k - b)2 = 0.01.
BQ    Aqr |d = 0.07P.
BR    Aqr |P var? (k - b)2 = 0.16.
BS    Aqr |Delta(S) = 0. P var?
BT    Aqr |B - V: +0.14, +0.52. P var. Blazhko effect.
BV    Aqr |P var. Blazhko effect with Pi =  11.56d and variations of
BV    Aqr |light in Max up to 0.75A.
BW    Aqr |d = 0.01P. Min II 10.8. Min II - Min I = 0.484P.
BW    Aqr |Jensch [00189] considers the secondary Min to be the
BW    Aqr |main one.
BX    Aqr |d = 0.027P.
CD    Aqr |d = 0.012P. Min II 10.2.
CE    Aqr |According to [02548], no
CE    Aqr |variations were found in visual observations during
CE    Aqr |several months in 1954 - 1958. According to [03138],
CE    Aqr |the star may be analogous to AI Vel; P = 0.16d?
CH    Aqr |P var?
CI    Aqr |Period may be twice as long.
CM    Aqr |Min II 13.6.
CP    Aqr |Delta(S) = 3.
CR    Aqr |Min II 14.2.
CV    Aqr |Minor planet (52) Europa.
CW    Aqr |Min II 10.8.
CX    Aqr |Min II 10.8. Broad hydrogen lines.
CY    Aqr |Delta(S) = 2. P var; abrupt change ~1952. Before JD2434000
CY    Aqr |Max = 2434308.4314 + 0.061038509d*E. The shape of
CY    Aqr |the light curve probably varies. For M - m different
CY    Aqr |authors give values from 0.23p to 0.40p. Beat phenomenon
CY    Aqr |with P2 = 0.2182d is possible [08060].
CZ    Aqr |Min II 11.1. Cyclic variations of period?
DD    Aqr |Min II 11.2.
DN    Aqr |(k - b)2 = 0.01.
DO    Aqr |P var.
DS    Aqr |P var.
DV    Aqr |Min II 6.1. SB. In [08061] variations were noted
DV    Aqr |with Delta(m) ~0.1m and P < 3h, presumably of DSCT
DV    Aqr |type nature. Some sources give A3 for the spectral
DV    Aqr |type. Shell spectrum was observed in May, 1975.
DV    Aqr |Spectral lines were filled with emission and therefore
DV    Aqr |weak, strong absorption in H and K CaII lines was present.
DV    Aqr |Shell effects were not present in the spectra taken in
DV    Aqr |1971 - 1973 [08062].
DX    Aqr |VB B (A 7.0m, K0III; B 3.7", 244deg). SB1. d ~0.015P.
DX    Aqr |Depth of Min II ~0.3m.
DX    Aqr |The range of combined brightness is given.
DY    Aqr |d = 0.04P.
EE    Aqr |Min II 8.48.
EK    Aqr |Min II 11.23.
EL    Aqr |P = 0.6345d is possible.
EM    Aqr |According to [06204] P = 0.068d.
EM    Aqr |Period and amplitude vary on very short time
EM    Aqr |scale. Light and colour vary approximately in phase.
EM    Aqr |The beat period, if exists, is shorter than 1d.
ET    Aqr |Period is given according to [08336].
EW    Aqr |Delta(m) varies.
FF    Aqr |d = 0.059P. SB1. The unique eclipsing system of a red
FF    Aqr |star and probably a blue hot subdwarf. The amplitude of
FF    Aqr |the eclipse is 0.15V, 0.4B, 1.2U. The magnitude in Max
FF    Aqr |varies by 0.35V, 0.33B, 0.22U. Variable shape of light
FF    Aqr |curve. Strong emissions H and K CaII, Halpha in the
FF    Aqr |spectrum.
FI    Aqr |Possibly P = 4.659d or 4.719d. Epoch of min is given.
FK    Aqr |BDS 11854 A (B = FL Aqr, 11.45m, 24", 352deg, 1966).
FK    Aqr |mu alpha = +0.455", mu delta =  -0.067". SB2 (P = 4.08322d
FK    Aqr |[00313]). Flares Delta(U) = 0.7 [00344].
FL    Aqr |BDS 11854 B (A = FK Aqr; B 24", 352deg, 1966).
KV    Aqr |One deep fading overlapping a brightening trend.
omi   Aqr |Shell or disk spectrum is observed.
pi    Aqr |The brightness increased by ~0.2m V
pi    Aqr |in 1957 - 1975, the star became redder. Balmer
pi    Aqr |continuum in emission. Rapid changes in emission
pi    Aqr |lines and in polarization. Existence of a disk
pi    Aqr |or a shell is possible.
R     Aql |P var. Max = 2440038 + 297d*E (JD2427850 - 40000).
R     Aql |Since JD2440000 - see Table.
R     Aql |For the whole observed period
R     Aql |Max = 2399190 + 346.932d*n - 0.239303d*n**2;
R     Aql |Pn = 348.980d - 0.554202d*n + 0.000552309d*n**2 [03143].
R     Aql |H2O, OH and SiO maser. Radiobursts.
U     Aql |B - V: +0.84, +1.24. P var. ADS 12503 A (B 14.00m,
U     Aql |35", 349deg, 1900; one more companion 11.7m V, 2", 230deg,
U     Aql |1934).
W     Aql |S 6/6e. Composite spectrum near Min light; a companion
W     Aql |(F5 - F8) may exist [03502].
Y     Aql |Depth of Min II 0.03m. SB1.
RR    Aql |Maser H2O, OH, SiO.
RT    Aql |Maser H20, OH, SiO.
SY    Aql |Maser H2O, OH.
SZ    Aql |B - V: +1.04, +1.82. P var [02392]. Before JD2420260
SZ    Aql |P = 17.1359d. Current elements - see Table.
TT    Aql |B - V: +0.96, +1.62. P var. [02392]. Before JD2418035
TT    Aql |P = 13.7518d.  Current elements - see Table.
TV    Aql |P var (changed at ~JD2430000).
TV    Aql |Before JD2430000 Max = 2429730 + 237.9d*E.
TW    Aql |Cycles 65d or 95d are observed during different time
TW    Aql |intervals [08714].
UU    Aql |Mean cycle: 71.3d [04063]; 56d [03144].
UY    Aql |Cyclic changes of light (P ~400d) with superimposed very
UY    Aql |rapid variations are noted in [00504].
VX    Aql |SC5-/8e. According to [04231], the variable is irregular.
VX    Aql |Lithium star.
VZ    Aql |B - V: +0.61, +1.01.
XZ    Aql |P var. Min = 2424449.277 + 2.139147d*E
XZ    Aql |(JD2424380 - 2430300). Since JD2433000 - see Table.
YZ    Aql |d = 0.03P. P var.
AA    Aql |Delta(S) = 1.0.
AC    Aql |P var.
AD    Aql |CN bands are observed in the spectrum. According to [06928],
AD    Aql |the range is 8.83 - 13.42 V.
AE    Aql |VB A (B 16.6m, 12", 330deg; C 16.9m, 11", 0deg).
AE    Aql |The combined light of A, B, C varies in the range
AE    Aql |13.9 - 15.8.
AF    Aql |The period may be two times shorter.
AL    Aql |d = 0.04P.
AU    Aql |According to [03146], P = 190d or 380d.
BL    Aql |P var. Max = 2418538 + 159.65d*E (JD2418529 -
BL    Aql |29075). During JD2436420 - 38940 - see Table.
BY    Aql |P var?
CD    Aql |Close companion?
CL    Aql |Sometimes maxima predicted according to the
CL    Aql |elements do not occur.
CM    Aql |Symbiotic spectrum similar to that of Z And [03149].
CR    Aql |Considerable Blazhko effect is possible.
CS    Aql |Close companion?
CT    Aql |According to [06004], only slow irregular variations with
CT    Aql |Delta(m) ~0.6 were observed in 1963 - 1968.
CU    Aql |P var? (Possible change ~JD2423000). Earlier Max = 2418591
CU    Aql |+ 203.7d*E.
CV    Aql |P var?
CW    Aql |Close companion?
DD    Aql |Close companion?
DT    Aql |P var (Change ~JD2425000). Earlier Max = 2423964 + 290.5d*E.
DY    Aql |P var [06107].
EV    Aql |P var. Before JD2423900 P = 38.67d. [A/H] = -0.3.
EX    Aql |P = 117d is also observed.
EZ    Aql |P var [06107].
FF    Aql |ADS 11884 A (B 10.37m, 7", 141deg). SB1 (P = 1435d).
FG    Aql |At the edge of the dark nebula Barnard 130. May be a
FG    Aql |physical pair with FH Aql (rho ~20"). According to
FG    Aql |[00504], the mean cycle of light variations is 3.5d.
FG    Aql |The level of mean light varies.
FH    Aql |At the edge of the dark nebula Barnard 130. May be a
FH    Aql |physical pair with FG Aql (rho ~ 20"). According to
FH    Aql |[00504], the mean cycle of light variations is 3.44d.
FK    Aql |Depth of Min II 0.03m. P var.
FM    Aql |B - V: +1.12, +1.50.
FN    Aql |B - V: +1.10, +1.39. P var.
FZ    Aql |VB A (B 11.5m, 14", 162deg).
GM    Aql |UV type is possible [00504].
GU    Aql |d = 0.02P.
GV    Aql |Nova-like star according to [02089].
GY    Aql |Maser OH, SiO.
HK    Aql |Type ISB is not excluded.
HL    Aql |P var? The 15m star shown in the charts [02274,06996] with
HL    Aql |co-ordinates coincident with those given at the discovery
HL    Aql |is constant according to [02274].
IM    Aql |P var. Before JD2432772 Max = 2428064.707 + 0.4569602d*E.
IO    Aql |VB A (B = IP Aql, 30", 101deg).
IP    Aql |VB B (A = IO Aql).
IS    Aql |Close companion.
KL    Aql |B - V: +0.78, +1.19, [A/H] = 0.6.
KO    Aql |d = 0.018P. Min II 8.40. P var. Min = 2427550.565 +
KO    Aql |2.863859d*E (JD2426250 - 33000) [02462]; Min =
KO    Aql |2433888.366 + 2.863954d*E (JD2433000 - 39000).
KO    Aql |current elements - see Table.
KP    Aql |Min II 10.43; Min II - Min I = 0.50P; DII = DI.
KV    Aql |During JD2429130 - 31370 - see Table.
KV    Aql |During JD2428308 - 28433 the star was faint. Max 2436015
KV    Aql |also is not satisfied by the elements.
LU    Aql |In [03158] P = 102d is given, and the existence of the
LU    Aql |variation of mean magnitude with P ~1080d and
LU    Aql |Delta(m) = 0.4m was suspected.
MV    Aql |Close component, the range is given for combined light.
NN    Aql |Cyclic P variations?
NV    Aql |Variations of mean light with P ~ 900d - 1000d and
NV    Aql |Delta(m) ~0.6m.
OO    Aql |Min II 9.8. P var. Min I = 2426892.0582 +
OO    Aql |0.5067954d*E (1932 - 1934), Min I = 2433925.3762 +
OO    Aql |0.5067943d*E [08072]. Since JD2438000 - see Table.
OO    Aql |The shape of the light curve varies.
OX    Aql |Var 2 in the chart for OW Aql.
PP    Aql |[A/H] = -0.0. CWA type
PP    Aql |is not excluded. According to [03161]
PP    Aql |P var. Max = 2415229.15 + 24.0147d*E (JD2415228 -
PP    Aql |21064), Max = 2426576.14 + 24.074d*E (JD2426576 -
PP    Aql |29489). After JD2432040 Max = 2433141.78 + 23.994d*E.
PP    Aql |Current elements Max = 2436836.04 + 23.973d*E.
PZ    Aql |P var? According to [05387], before JD2428075 P = 8.7555d;
PZ    Aql |P = 8.7504d (JD2428075 - 34725); since JD2434725
PZ    Aql |P = 8.7573d. See also [02274]. Elements in the Table are
PZ    Aql |satisfactory after JD2433150. The shape of the light curve
PZ    Aql |apparently varies.
QS    Aql |Min II 5.97. VB (A 6.5m; B 6.7m, 0.18", 137deg). P var.
QV    Aql |The epoch of main Max is given.
QY    Aql |d = 0.016P. P var?
V0336 Aql |B - V: +1.17, +1.55.
V0337 Aql |Min II 9.09. P var.
V0337 Aql |The shape of the light curve varies.
V0340 Aql |d = 0.05P. P var.
V0341 Aql |P var. Delta(S) = 4.
V0342 Aql |ADS 12259 B (A 7.5m; B 20", 14deg); d = 0.032P. P
V0342 Aql |increases (see also [02265,04493]). Before JD2435600 Min =
V0342 Aql |2428023.550 + 3.390842d*E.
V0342 Aql |Halpha emission observed at Max light [08074]. The shape
V0342 Aql |of the light curve and d apparently vary. Delta(m)
V0342 Aql |probably decreases [08075].
V0343 Aql |Min II 10.7.
V0346 Aql |Min II 9.1. ADS 13438 A (B 11.3m, 2", 245deg).
V0346 Aql |Elements in the Table are valid after
V0346 Aql |JD2437000. The shape of Min I varies [07001].
V0348 Aql |d ~0.08P.
V0352 Aql |The nucleus of the supposed planetary nebula P.K.
V0352 Aql |37-3.3deg.
V0356 Aql |VB A (B 0.2").
V0367 Aql |The elements are satisfactory
V0367 Aql |only during JD2436450 - 37960. Resembles S Vul.
V0368 Aql |VB A (B 0.17", 140deg).
V0374 Aql |VB A (B ~0.2',  ~270deg).
V0406 Aql |Min II 13.3:.
V0407 Aql |P var; there is a nonlinear term in the elements:
V0407 Aql |+1.51d*10**(-9)*E**2.
V0409 Aql |Min II 12.2. Spectral type from another publication
V0409 Aql |is A2 - A3.
V0411 Aql |Epoch of Min is given.
V0417 Aql |Min II 11.5. P var. Before JD2439000:
V0417 Aql |Min = 2428427.127 + 0.3701251d*E.
V0421 Aql |P var?
V0423 Aql |Elements are valid for JD2426900 - 28000. During
V0423 Aql |JD2429020 - 31670 the waves are much longer or absent.
V0433 Aql |Waves of 26d - 80d duration with Delta(m) = 0.1m - 0.9m.
V0433 Aql |The mean light varies according to the formula
V0433 Aql |Max = 2438312 + 648d*E.
V0449 Aql |The star in [01091,02282] is actually not identical to HV5424.
V0461 Aql |Close component ~15.5m, the range of combined light is
V0461 Aql |given.
V0467 Aql |Waves of 40d - 72d duration. The mean light varies with
V0467 Aql |P ~1400d.
V0473 Aql |P ~330d is sometimes observed.
V0476 Aql |EW type with doubled period is possible. Elements are based
V0476 Aql |on a short series of observations.
V0483 Aql |In the field of the open cluster NGC 6709.
V0486 Aql |In the field of the open cluster NGC 6709.
V0493 Aql |B - V: +1.10, +1.38.
V0495 Aql |d = 0.06P:.
V0496 Aql |B - V: +1.07, +1.28. Elements are given for epochs after
V0496 Aql |JD2428000.
V0497 Aql |VB A (B 16.5m, 9",  ~0deg).
V0524 Aql |The variable is np from the star shown in the chart
V0524 Aql |in [02317].
V0527 Aql |IS type is possible.
V0528 Aql |VB A (B 16.5m, 11", 59deg).
V0535 Aql |VB [01943], two components are seen on Palomar prints,
V0535 Aql |eastern of them being red. According to [01943], rapid
V0535 Aql |variable.
V0537 Aql |Possible P = 200d.
V0538 Aql |Possible P = 375d.
V0558 Aql |Possible P = 187d.
V0571 Aql |Possible P = 185.5d.
V0572 Aql |B - V: +0.65, +0.87. P var. Before JD2435500 P ~3.7686d.
V0572 Aql |See also [08637]. JD2433631.8421 + 0.716292d*E.
V0572 Aql |See also [02124].
V0586 Aql |Irregularities are sometimes observed, but then the
V0586 Aql |periodicity is probably resumed.
V0596 Aql |Resembles S Vul.
V0599 Aql |Min II 6.73. According to [08083], may be constant.
V0600 Aql |B - V: +1.36, +1.70.
V0600 Aql |Before JD2428000 another value of P is possible [08632].
V0602 Aql |d = 0.02P. Min II 12.7.
V0603 Aql |SB (P = 0.13854d [03169]). Outside the outburst there are
V0603 Aql |variations of light (eclipses) with Delta(m) = 0.30m,
V0603 Aql |Min I = 2444401.399 + 0.1377d*E (D ~0.2P). The
V0603 Aql |shape of the light curve and the depth of minima differ
V0603 Aql |from cycle to cycle. The brightness in minima shows
V0603 Aql |fluctuations apparently connected with the presence of
V0603 Aql |a hot spot [04500].
V0605 Aql |A unigue variable. 8" np from a 17m star. Min ~20m pg.
V0605 Aql |Photographs of the field [06041,06042]. The
V0605 Aql |light curve resembles those of the SN in NGC
V0605 Aql |1058 or of eta Car [06040]. The only Max observed, with
V0605 Aql |fluctuations, occured in 1918 - 1924. In 1921 the spectral
V0605 Aql |type was found to be R [02464]. The star is inside the old
V0605 Aql |planetary nebula A 58 and may be its nucleus.
V0609 Aql |Min II 11.9.
V0615 Aql |P var? Max = 2428046 + 364d*E (JD2428038 - 31343) [01091].
V0616 Aql |d = 0.04P. Elements reguire verification.
V0618 Aql |Twice shorter period is not excluded.
V0637 Aql |Twice shorter period is not excluded.
V0638 Aql |Twice shorter period is not excluded.
V0640 Aql |Min II 12.8.
V0647 Aql |Slight Min II [01091].
V0663 Aql |P = 194.5d is possible.
V0666 Aql |The range is given for combined magnitude with a preceding
V0666 Aql |16.5m star. Separately was found ~17m pg near Min.
V0672 Aql |P var? Blazhko effect is possible [03113].
V0678 Aql |P var. Before JD2429723 Max = 2429723 + 120.6d*E.
V0688 Aql |Min II 10.8. DII = 0.15P.
V0694 Aql |d = 0.13P. VB (1"), a companion ~1m fainter than
V0694 Aql |the variable [01881] may have affected the data given.
V0699 Aql |Min II 13.75.
V0706 Aql |Delta(S) = 0:.
V0708 Aql |P ~65d waves superimposed on slow variation of mean
V0708 Aql |brightness with P ~1350d (JD2437124 - 40512) [06025].
V0708 Aql |According to [00773] waves with P ~100d - 150d
V0708 Aql |(JD2427543 - 31318).
V0714 Aql |d = 0.05P.
V0724 Aql |Min II 11.57.
V0733 Aql |P var? Before JD2434500,
V0733 Aql |possibly Max = 2434453.72 + 6.17687d*E [00001].
V0734 Aql |VB A? (B 16.1m?).
V0743 Aql |White. SRD?
V0755 Aql |Alternative elements: Min = 2429195.290 + 1.01598d*E.
V0765 Aql |B - V: +0.70, +0.80.
V0766 Aql |EW type is not excluded.
V0769 Aql |d = 0.05P?
V0770 Aql |Min II 14.0.
V0771 Aql |According to [03165] UG.
V0774 Aql |Possibly resembles UV Boo.
V0777 Aql |P = 111.5d is possible.
V0784 Aql |Min II 14.8.
V0794 Aql |Rapid changes with Delta(m) up to 1.5m superimposed on
V0794 Aql |slow ones. May belong to "polars" of XPRM type. Peculiar
V0794 Aql |spectrum with broad emissions and blue continuum [08676].
V0800 Aql |VB. According to [06072] UGZ.
V0801 Aql |VB A (B 15.1m sp).
V0803 Aql |Min II 14.8.
V0804 Aql |Min II 12.8. In Max B - V = +0.61.
V0805 Aql |Min II 7.90, DII = 0.11P.
V0808 Aql |Min II 13.3.
V0812 Aql |VB A (B 16m sp, C 16m sf).
V0814 Aql |VB A (B 16.5m sp).
V0822 Aql |Min II 7.07. ADS 12538 A (B 10.1m, 1", 67deg). The shape
V0822 Aql |of the light curve varies.(U - B) index in Min I is redder
V0822 Aql |and Min II is bluer than average.
V0829 Aql |Twice longer P is possible.
V0836 Aql |RR type is possible ([00085]; it is suggested also by the
V0836 Aql |spectrum [08676]).
V0850 Aql |In the centre of the planetary nebula P.K. 37-6.2.
V0866 Aql |Min II 14.8. According to [06026], the depth
V0866 Aql |of Min II 0.4m, EB type.
V0867 Aql |P var?
V0871 Aql |Min II 14.5, Min II - Min I = 0.425P.
V0871 Aql |Physical changes in the range 13.3 - 13.6 are
V0871 Aql |possible. Eclipses start from the 13.6m level.
V0872 Aql |Min II 15.7:. Apsidal motion is possible.
V0873 Aql |P var? The mean light varies in the range 13.8 - 14.0.
V0875 Aql |White. According to [06004], rapid. Possibly UGZ or IA.
V0877 Aql |VB A (B 16.5m nf).
V0882 Aql |Blazhko effect is possible.
V0885 Aql |Min II 14.9:. Apsidal motion and changes of the shape of
V0885 Aql |the light curve are possible.
V0888 Aql |A possible member of the open cluster NGC 6738.
V0889 Aql |Min II 9.0. Min II - Min I = 0.35P.
V0889 Aql |Apsidal motion is possible.
V0890 Aql |Nova Aql 1946 = asteroid N258 Tyche [09038].
V0891 Aql |Min II 15.8.
V0895 Aql |P var. Max = 2430931.435 + 0.265108d*E
V0895 Aql |(JD2426920 - 35010) [02267].
V0895 Aql |During JD2441890 - 42290 - see Table.
V0907 Aql |Min II 15.7.
V0912 Aql |The shape of the light curve varies.
V0914 Aql |P = 3.336217d
V0914 Aql |is given in [08717] by misprint.
V0919 Aql |Min II 13.8.
V0920 Aql |F or earlier observations Max = 2429458.400 + 0.4955033d*E.
V0922 Aql |Elements are not quite reliable.
V0923 Aql |Unusual shell star [01884]. Similar to EW Lac.
V0923 Aql |He lines are widened by the rotation, NaI lines
V0923 Aql |are narrow. Light changes are periodic: Min =
V0923 Aql |2436458.66 + 0.8518d*E. The cause of variations is
V0923 Aql |probably connected with the rotation and the inhomogeneous
V0923 Aql |brightness distribution over the disk of the star [03178].
V0923 Aql |Profiles of spectral lines vary. The expansion of the
V0923 Aql |envelope terminated in 1965, which apparently led to the
V0923 Aql |development of inhomogeneities and to the broadening of
V0923 Aql |hydrogen line profiles [04525].
V0925 Aql |Some observers found constant brightness [03165].
V0929 Aql |Short period.
V0936 Aql |Short period.
V0947 Aql |According to [05412], rapid irregular
V0947 Aql |changes are not excluded. According to [00504], constant.
V0955 Aql |Min II 14.9, DII = 0.13P.
V0956 Aql |Min II 14.2. Elements need confirmation.
V0957 Aql |P var. Max = 2428154.960 + 0.6051327d*E
V0957 Aql |(JD2421871 - 28105).
V0958 Aql |VB A (B 17.0m, 0.2' np; C slightly brighter, 0.1'f).
V0958 Aql |Combined magnitude of A and C is given.
V0964 Aql |Min II 13.7.
V0969 Aql |Blazhko effect is possible.
V0981 Aql |Min II 14.5.
V0991 Aql |IS type is possible.
V0992 Aql |According to [04260], P = 110d.
V0998 Aql |The position coincides with the planetary nebula
V0998 Aql |P.K.50-3.1deg.
V0999 Aql |Tsessevich's observations [07806] do not agree with the
V0999 Aql |elements in the Table.
V1017 Aql |Elements need confirmation.
V1033 Aql |P var?
V1045 Aql |Min II 13.5.
V1046 Aql |P var? [08321].Min = 2427713.314 + 5.28303d*E [04027].
V1046 Aql |Slight reflection effect is possible.
V1064 Aql |Cycles 295d - 410d.
V1072 Aql |sp component of a close pair.
V1075 Aql |d = 0.04P. Min II 13.6.
V1076 Aql |VB A (close preceding).
V1086 Aql |VB. Probably the variable is the sf component.
V1093 Aql |IA type is possible.
V1095 Aql |P var. After JD2429048 - see Table, earlier
V1095 Aql |Max = 2427322 + 42.68d*E. Not coloured appreciably.
V1096 Aql |Min II 13.3.
V1097 Aql |Min II 14.0.
V1101 Aql |Possibly UGZ type [03156].
V1113 Aql |The period may be twice shorter.
V1117 Aql |Min II 16.6.
V1125 Aql |Min II 16.0.
V1140 Aql |P var?
V1154 Aql |Min II 14.8; Min II - Min I = 0.70P.
V1165 Aql |According to [04564], constant. In [03932] was not separated
V1165 Aql |from a close component which probably led to distortions
V1165 Aql |of the light curve.
V1166 Aql |UG type is possible.
V1173 Aql |nf component of a close pair.
V1182 Aql |Min II 8.65.
V1184 Aql |Min II 13.4.
V1200 Aql |VB. The variable is the eastern red component.
V1204 Aql |VB. The variable is the eastern component.
V1208 Aql |A common proper motion star 9.06m in 1' to the south.
V1248 Aql |UG type is possible.
V1251 Aql |Red.
V1261 Aql |Spectral type K2 in HD.
V1269 Aql |VB. The variable is the preceding component.
V1281 Aql |Reddish. SRD type is possible.
V1286 Aql |Possibly the period is accidental.
V1288 Aql |ADS 12182 A (B 12.3m, 36", 287deg).
V1291 Aql |The elements have been determined on the base of magnetic
V1291 Aql |field variations. The epoch of minimum intensity of the
V1291 Aql |magnetic field is given.
V1295 Aql |Shell star. Dramatic spectral changes were observed [05240].
V1295 Aql |The variability is hardly periodic, though P ~100d is
V1295 Aql |possible. Sometimes light fluctuations on several days'
V1295 Aql |time scale are observed [05880]. IR excess [06277]. For a
V1295 Aql |detailed spectroscoric study, with evidence for the
V1295 Aql |outflow of matter from the surface, see [04739].
V1295 Aql |Considerable magnetic field [04435].
V1297 Aql |d = 0.05P? Min II 14.5.
V1298 Aql |mu alpha = -0.0392s,  mu delta = -1".330.
V1298 Aql |The companion of the star BD +4deg 4048 (ro =
V1298 Aql |73".8, theta = 151.5 deg).
V1298 Aql |One of the absolutely faintest known stars (Mv = +19m).
V1300 Aql |I - K: +5.2, +6.5. Sometimes CO, SiO, OH maser emission.
V1302 Aql |A unique IR object IRC +10420. B - V = +2.7, U - B = +1.9.
V1302 Aql |OH, H2O, SiO maser. According to [07437], the energy
V1302 Aql |distribution in the IR spectrum (1 - 22mkm) resembles that
V1302 Aql |of eta Car. Emissions of neutral metals are observed in
V1302 Aql |the spectrum. Increased in brightness during 1925 - 1970;
V1302 Aql |Max ~1970.
V1323 Aql |Close VB; var - northern component.
V1325 Aql |VB, np component var.
V1331 Aql |Min II 7.95. According to [04619] P = 1.364076d.
V1333 Aql |Aql X-1. Light variations with P ~1.28d - 1.31d due to
V1333 Aql |orbital motion are possible [04625]. Bursts characteristic
V1333 Aql |of the XB type are observed [04757]. Lx/Lopt ~500 outside
V1333 Aql |nova-like bursts, Lx/Lopt ~5000 during bursts.
V1336 Aql |In 1.6' W from MXB 1916-05. M type is possible.
V1338 Aql |VB. Probably the f component, very bright infrared, is var.
V1340 Aql |d = 0.06P? Intrinsic lightvariations in Max are possible.
V1341 Aql |Min II 13.4. P = 0.3586768D is possible.
V1343 Aql |SS 433. <B - V> = +2.0. Associated with the SNR W 50. Mean
V1343 Aql |light varies in the range 14.0 - 14.6 V according to the
V1343 Aql |elements Max = 2443662.5 + 165.5d*E [00512]. The depth of
V1343 Aql |Min I varies from 0.2m to 0.9m V, the depth of Min II
V1343 Aql |varies from 0 to 0.4m V. Two systems of H, HeI, HeII
V1343 Aql |emission lines are observed in the spectrum: the
V1343 Aql |"stationary" system corresponding to Vr changes from 300
V1343 Aql |to 150 km/s with P = 13.1d, and the "relativistic" one,
V1343 Aql |corresponding to Vr changes from +50000 to -35000 km/s
V1343 Aql |with P = 165.5d. The spectral study [00535]. The system
V1343 Aql |apparently consists of an O - B star filling its inner
V1343 Aql |Roche lobe and a compact object surrounded by an accretion
V1343 Aql |disc wich is precessing with P = 165.5d. Two jets
V1343 Aql |consisting of dense condensations of matter emerge from
V1343 Aql |the system with relativistic velocity (0.27 c) in opposite
V1343 Aql |directions. The luminosity of the disc amounts to not less
V1343 Aql |than 60% of the total luminosity of the system [00926,00953].
V1343 Aql |The object may be a former supernova which bursted not
V1343 Aql |more than 10**4 years ago.
V1345 Aql |Min II 14.3:, Min II - Min I = 0.46P.
V1349 Aql |Max ~17 pg.
V1352 Aql |VB A (B 14.5m, 6", 175deg).
V1353 Aql |Min II 10.9.
V1355 Aql |Min II 13.3.
V1357 Aql |Possibly P = 1.051d.
V1470 Aql |The variability may be due to the fainter (B) component.
V1472 Aql |SB, Porb = 198d.
V1648 Aql |Brightening over 10 years, probably due to dissipating dust envelope,
V1648 Aql |plus quasi-periodic variations.
eta   Aql |P var. P = 7.176344d (JD2373000 - 95100),
eta   Aql |P = 7.176455D (JD2395100 - 2412100). Since JD2412100 -
eta   Aql |see Table. For the whole interval
eta   Aql |Max = 2442794.773 + 7.176735d*E + 2.18d*10**(-8)*E**2
eta   Aql |[08632]. In the UV band the light of a possible A0V
eta   Aql |comparion is apparent.
sig   Aql |ADS 12737 A (B 12.34m, 48", 328deg). Depth of Min II 0.1m.
sig   Aql |In [04627] P = 1.950271d is given according to
sig   Aql |spectroscopic data.
R     Ara |Min II 6.2. VB A (B 8.2mV,  4", 123deg).
S     Ara |(k - b)2 = 0.09. P var [01932,03126]. Max = 2416284.792 +
S     Ara |0.45188910d*E (JD2414000 - 19000);Max =
S     Ara |2419149.797 + 0.45188581d*E (JD2419000 -
S     Ara |30000) [00752]. Since JD2441000 - see Table. For the
S     Ara |whole interval, with sufficient accuracy,
S     Ara |Max = 2420047.2382 + 0.451888176d*E - 1.36d*10**(-10)*E**2
S     Ara |[03126].
T     Ara |VB A (B 11.0m, 34", 60deg).
X     Ara |Shown in the chart for S5809.
RT    Ara |According to Cannon [01944] who discovered the star's
RT    Ara |variability, a companion 12.0m is present in 0.1m to W
RT    Ara |and somewhat to the north from the variable. Cannon points
RT    Ara |out that at Min light the variable becomes fainter than
RT    Ara |the companion. No sign of the companion's existence was
RT    Ara |found by Hoffmeister [00016] and by Payne-Gaposchkin [00624].
RT    Ara |According to [00624], the mean cycle is ~78d, and RVA
RT    Ara |type is possible.
RW    Ara |d = 0.022P. Min II 8.91. Changes of the shape of the light
RW    Ara |curve due to gaseous streams or a hot spot are possible.
TT    Ara |ZrO bands may be present in the spectrum [03181].
TV    Ara |In the region of the cluster NGC 6208.
TX    Ara |VB A (B 16.5m). Twice shorter period is possible.
XX    Ara |Min II 14.1.
YY    Ara |The star's being an eclipsing or irregular variable is not
YY    Ara |excluded [00424].
AA    Ara |Min II 13.3.
AD    Ara |[A/H] =  -0.4.
AE    Ara |VB A (B 12m, 0.3' sf). P.K. 344-8.1.
AE    Ara |A compast planetary nebula or a symbiotic star. Irregular
AE    Ara |abrupt brightenings by 3m - 4m separated by several years
AE    Ara |are observed [00255]. The spectral data are discussed in
AE    Ara |[08076].
AF    Ara |Min II 13.8.
AW    Ara |Before JD2417300 Max = 2412600 + 186d*E.
BQ    Ara |Double maxima separated by 10d - 20d, with Min II 12.8.
CC    Ara |VB; the variable is nf component.
CH    Ara |Noted on the finding chart for S6062 = V 466 Ara.
CT    Ara |Before JD2420400 Max = 2413080 + 215d:*E;
CT    Ara |since JD2425000 - see Table.
DU    Ara |B - V: +0.52, +0.84. P var. Max = 2418145.560 +
DU    Ara |1.63999d*E (JD2411000 - 21000); Since
DU    Ara |JD2425000 - see Table.
EK    Ara |VB A (B 15m).
EL    Ara |Before JD2420400 Max = 2415140 + 332d*E;
EL    Ara |since JD2425000 - see Table.
ER    Ara |Min II 14.2.
EV    Ara |Before JD2420400 Max = 2413750 + 237d*E;
EV    Ara |since JD2425000 - see Table.
EZ    Ara |P var.
FU    Ara |The depth of Min I is 0.97m and 0.89m,
FU    Ara |the depth of Min II is 0.20m and 0.23m in blue and
FU    Ara |yellow light, respectively.
GK    Ara |Before JD2417800 Max = 2414050 + 237d*E,
GK    Ara |since JD2418400 - see Table.
GM    Ara |Min II 12.8.
HX    Ara |B - V: +0.23, +0.36. A hump on the ascending branch
HX    Ara |(phi = 0.93P) [08118].
KY    Ara |Only one sharp Max (JD2428715 - 712) was observed.
KY    Ara |Possibly a Nova.
KZ    Ara |VB A (B 14.1m sp).
LP    Ara |d = 0.04P? Min II 10.5?
LQ    Ara |In 1959 rapid variations at times for 0.5m near 11m
LQ    Ara |were observed; surrounded by a nebula [04001].
LR    Ara |Min II 10.6.
LU    Ara |Min II 10.1?
MQ    Ara |nf component is variable.
MR    Ara |B - V: +0.72, +0.8. [A/H] =  -1.0. P var?
QR    Ara |Shown in the charp for BV 1443.
QU    Ara |VB.
QW    Ara |The variable is np component of the pair.
QX    Ara |Shown in the chart for S5818.
V0340 Ara |B - V: +1.25, +1.68. [A/H] = 0.6.
V0341 Ara |The star is blue; light variations during 4d were not
V0341 Ara |accompanied by colour changes. Possibly an eclipsing
V0341 Ara |variable [04678].
V0342 Ara |P >= 140d.
V0344 Ara |P >= 170d
V0345 Ara |P >= 180d.
V0349 Ara |Min II 8.8.
V0355 Ara |P > 220d.
V0356 Ara |P > 170d.
V0357 Ara |P >= 220d.
V0360 Ara |Min II 13.8:, Min II - Min I = 0.35P.
V0361 Ara |Min II 13.6:.
V0362 Ara |Min II 15.6:.
V0383 Ara |A star 16.5m is close to the north.
V0421 Ara |Min II 15.1.
V0440 Ara |Min II 14.5:.
V0444 Ara |Min II 14.2.
V0454 Ara |Min II 14.1.
V0480 Ara |Min II 15.5:.
V0484 Ara |RV type is possible (Min = JD2436760).
V0485 Ara |Min II 14.8.
V0489 Ara |Min II 11.9.
V0491 Ara |Min II 11.9.
V0492 Ara |Min II 14.5.
V0494 Ara |RV type is not excluded.
V0501 Ara |Min II 13.8. Shown in the chart for S6114.
V0535 Ara |Min II 7.71. Nonlinear term in the elements:
V0535 Ara |-4.4d*10**(-11)*E**2.
V0536 Ara |Min II is present. EB type is possible. P var.
V0536 Ara |P = 2.374101d (JD2415000 - 22000); since JD2422000 -
V0536 Ara |see Table.
V0539 Ara |VB A (B 9.22m, 12", 269deg). Min II 6.09, d = 0.01P.
V0539 Ara |Shown in the chart for BV1441 = V538 Ara.
V0544 Ara |14.5m star sp.
V0609 Ara |Shown in the chart for S5867.
V0610 Ara |EA type is possible.
V0613 Ara |VB (close np companion is NSV10198).
V0616 Ara |Deep Min II.
V0620 Ara |Min II is possibly present.
V0623 Ara |Min II 14.5. Twice shorter period is possible.
V0624 Ara |P >= 220d.
V0625 Ara |P >= 170d.
V0639 Ara |V1 (NGC 6397). Probably not a cluster member.
V0651 Ara |Min II 15.3.
V0653 Ara |Min II 12.6.
V0656 Ara |EW type is not excluded.
V0658 Ara |Min II 16.0.
V0659 Ara |Min II 14.4.
V0668 Ara |Min II 13.8:.
V0675 Ara |P >= 200d.
V0687 Ara |RRC type is possible.
V0700 Ara |Min II 15.7.
V0702 Ara |Min II 14.0.
V0704 Ara |Min II 13.3.
V0705 Ara |Min II 14.4. RR type is possible.
V0716 Ara |Monotonous brightening during JD2436689 - 36838 was
V0716 Ara |found. The amplitude is probably greater.
V0722 Ara |Min II 10.3:.
V0728 Ara |Min II 12.8.
V0732 Ara |CEP type is not excluded.
V0743 Ara |RV type is possible.
V0781 Ara |Min II 14.8:.
V0783 Ara |Min II 13.9:.
V0785 Ara |Min II 14.3.
V0787 Ara |RV type is possible. Min JD2436756.
V0789 Ara |Min II 14.8.
V0790 Ara |Min II 14.8.
V0791 Ara |Min II 13.0:.
V0792 Ara |Min II 15.2:.
V0801 Ara |MXB 1636-53. Description of the spectrum [01356].
V0801 Ara |Modulation with P ~4h and the amplitude up to 40% was
V0801 Ara |found in the broad band optical flux [04944].
V0802 Ara |14.93 - 17.03 B.
V0808 Ara |EW type is possible.
V0820 Ara |Epoch of Min is given. Strong magnetic field. Either an
V0820 Ara |eclipsing binary or (more probably) an object similar to
V0820 Ara |rotating variables of ACV type.
V0821 Ara |4U 1658-48. Unusua1 X-ray system. Quasiperiodic optical
V0821 Ara |variations (P ~20s) with total amplitude 40 percent,
V0821 Ara |abrupt bursts on ~20 ms time scale leading to two-fold
V0821 Ara |flux increase and light changes by 6m during less than
V0821 Ara |two months were observed [04958]. Lx/Lopt = 3.
V0870 Ara |Type DSCT: is also possible.
R     Ari |OH emission.
T     Ari |P var. Max = 2417160 + 313.5d*E (JD2404800 -
T     Ari |17200); Max = 2434616 + 323.1d*E (JD2419400 -
T     Ari |34560). Since JD2436560 - see Table. <P> = 319.53d
T     Ari |(JD2404800 -  44160). Sometimes A < 1.5m.
U     Ari |SiO maser.
V     Ari |Vr =  - 180 km/s.
W     Ari |Maps given in [02544,06067] are wrong.
X     Ari |B - V: +0.28,  +0.56. P var. Max = 2420785.635 +
X     Ari |0.6511248d*E (JD2420460 - 33210) [03506]. Since
X     Ari |JD2433210 - see Table. [Fe/H] = -2.17.
RR    Ari |Min II 6.75:; Min II - Min I = 0.55P. Variability is not
RR    Ari |confirmed by other authors' photoelectric observations.
RR    Ari |V = 5.75.
RS    Ari |Min II 11.0.
RU    Ari |OH emission.
RV    Ari |B - V: +0.29,  +0.44. 0.34P =< M - m =< 0.53P.
RV    Ari |P1 = 0.07195d [08137]; P2 = 0.27554d [07033]. Moments of
RV    Ari |brightest light maxima T = 2435066.400 + 0.31632996d*n
RV    Ari |[02290].
RW    Ari |B - V: +0.35,  +0.46. P var. Max = 2428183.324 +
RW    Ari |0.3543184d*E (JD2428040 - 36700) [03188]. Since
RW    Ari |JD2440900 - see Table. According to [06043] - EA type:
RW    Ari |Min I = 2439384.97 + 3.1754d*E. Total light range
RW    Ari |(11.47 - 13.25 V) [08127] seems doubtful. It is not
RW    Ari |excluded that the eclipses and light increase of RW Ari
RW    Ari |given in [08127] are explained by variability of one of
RW    Ari |comparison stars used.
RX    Ari |d = 0.02P. Depth of Min II 0.10m.
SS    Ari |P var. Min II 10.82:.
ST    Ari |P var. Max = 2427347 + 94.2d*E (1933 - 1939); Max =
ST    Ari |2429525 + 106.6d*E (1939 - 1942); Max = 2430588 +
ST    Ari |95.2d*E (1942 - 1946); Max = 2432118 + 100.0d*E
ST    Ari |(1946 - 1961). Mean elements are given in the Table.
SX    Ari |B - V: -0.10,  -0.12. Epoch of Min is given.
SZ    Ari |d = 0.03P.
TT    Ari |Porb = 0.137551d [08138]. Along with light variations
TT    Ari |typical for Z Cam variables there are sinusoidal variations
TT    Ari |with amplitude of about 0.2m B and variable period:
TT    Ari |P = 0.1329d (1961 - 62), P = 0.1327d (1966) [04931],
TT    Ari |P = 0.1326d (1978) [04935]. Sinusoidal variations are
TT    Ari |superimposed by quasiperiodic oscillations up to 0.2m with
TT    Ari |8 - 20 minutes cycle and irregular flickering up to 0.1m
TT    Ari |in 1 minute.
TU    Ari |P var. Max = 2420463.353 + 0.4716219d*E
TU    Ari |(JD2420463 - 34720). Since JD2436820 - see Table.
TV    Ari |P var.
TX    Ari |P var?
TY    Ari |Form of the light curve varies. Mean value of the period
TY    Ari |is given.
UV    Ari |The second overtone period given in the
UV    Ari |Table is dominating. Sometimes the fundamental
UV    Ari |period P0 = 0.062d and the first overtone period P1 =
UV    Ari |0.047d are observed.
UW    Ari |Amplitude varies. In the interval JD2441581 - 693 - const.
UW    Ari |[07544].
UX    Ari |T = 2440133.766 + 6.43791d*E [06444], where T is epoch of
UX    Ari |conjunction (G5 component is behind K0 component).
UX    Ari |Brightness varies in waves with a period ~Porb, but the
UX    Ari |phase psi of light minimum calculated according to the
UX    Ari |elements given above changes with time: psi = 0.1P
UX    Ari |(1972 - 1974), psi = 0.8P (1976), psi = 0.7P (1977),
UX    Ari |psi = 0.6P (1978). Mean brightness varies, amplitude of
UX    Ari |the wave varies from 0.04m up to 0.15m.
VW    Ari |BDS 1269 A (B 8.33m, 74", 31deg). P2 = 0.089d.
VW    Ari |Metal deficiency. The companion has normal metal abundance.
VY    Ari |SB? Epoch of Min is given.
VY    Ari |Second light variation is also observed: Min =
VY    Ari |2442044.6 + 43.9d*E. A small flare in U band was
VY    Ari |observed.
gam   Ari |VB A (B 4.65m, B 9 V, 7.9", 0deg). Epoch of Min is given.
R     Aur |VB A (B 8.6m, 48", 239deg). P var [07165];
R     Aur |cycle 64.5a is possible.
S     Aur |P var. In the early fourties of our century the star was
S     Aur |faint with small and irregular variations.
T     Aur |Min = 2437614.0088 + 0.20437851d*E [08145]. P var?
T     Aur |<V> = 14.92, <B - V> =  + 0.28. There are light
T     Aur |fluctuations between the eclipses. Depths of Min are
T     Aur |0.10m - 0.28m [03195]. Faint nebula with high degree of
T     Aur |ionization.
U     Aur |H2O maser.
Y     Aur |B - V: +0.70,  +1.06.
Z     Aur |P var [07110]. Max = 2425580 + 110.76d*E
Z     Aur |(JD2416156 - 25580); Max = 2429888 + 113.35d*E
Z     Aur |(JD2425570 - 29900); Max = 2438292 + 135.55d*E
Z     Aur |(JD2429900 - 33300). P = 110d (1965) [03196].
Z     Aur |In 1970 - irregular variations [07338]. <V> =  -165 km/s;
Z     Aur |According to TiO bands the spectrum is M1 [00806].
RS    Aur |P var.
RT    Aur |B - V: +0.39,  +0.80. [A/H] = 0.1. P var. Max =
RT    Aur |2433040.867 + 3.728365d*E (JD2417970 - 33100).
RT    Aur |Since JD2433100 - see Table. Delta(V) var?
RU    Aur |OH emission.
RU    Aur |Mean magnitude probably varies with Pi = 10400d [01059].
RW    Aur |VB A (B 12.5m, dM0e, 1.2", 254deg).
RW    Aur |The companion probably flares with an amplitude
RW    Aur |0.5m - 0.7m [03197,03198]. Possible period of axial
RW    Aur |rotation is 100d [07067]. OH emission.
RX    Aur |B - V: +0.76,  +1.18; [A/H] =  -0.1, P var?
RX    Aur |Nonlinear term: -0.70d*10**(-6)E**2?
RZ    Aur |P var. Min = 2422616.498 + 3.010593d*E
RZ    Aur |(JD2418000 - 26000); since JD2426000 - see Table.
SS    Aur |SB (P = 0.1805939d [06103]).
SS    Aur |Sometimes abnormal behaviour of the star is
SS    Aur |being observed when comparatively numerous and
SS    Aur |small light maxima arise. According to [08151] the
SS    Aur |mean cycle is 51.2d.
SU    Aur |Common proper motion with AB Aur (P = 3'). Associated
SU    Aur |with a small bright nebula. OH emission.
SX    Aur |Min II 8.87. According to [08153] P var:
SX    Aur |Min I = 2418218.7779 + 1.21007653d*E + 0.91d*10**(-10)*E**2.
SY    Aur |B - V: +0.92,  +1.23. [A/H] =  - 0.3. P var [05661].
SY    Aur |Max = 2436853.57 + 10.144330d*E (JD2417900 -
SY    Aur |32380). Since JD2432380 - see Table.
TT    Aur |Min II 9.0.
TV    Aur |S5/6-.
TW    Aur |Mean magnitude varies with P = 1370d.
TZ    Aur |B - V: +0.08,  +0.48. Delta(S) = 2.
UU    Aur |VB A (B 11m, 18", 222deg).
UV    Aur |VB A (B 10.96m, B 9 V, 3.4", 4deg).
UV    Aur |Bright lines [NeIII] and [OIII] in spectrum.
UW    Aur |Epoch of Min is given.
UY    Aur |VB A (B 12m?, 0.8", 212deg). OH emission.
VW    Aur |VB (9.0m, 11.8m, 1.4", 332deg, 1976).
VX    Aur |P var?
WW    Aur |Min II 6.43. Min II - Min I = 0.50P.
XX    Aur |Min II 13.4.
YZ    Aur |B - V: +1.15,  +1.72. [A/H] =  -0.4.
ZZ    Aur |Min II 11.1.
AB    Aur |Common proper motion with AB Aur (P = 3'). Associated
AB    Aur |with a small bright nebula. OH emission. Spectrum
AB    Aur |description [04002].
AE    Aur |Connected with the bright nebula IC
AE    Aur |405. The motion is directed away from Ori OB 1
AE    Aur |association with the velocity 106 km/s.
AG    Aur |According to TiO bands
AG    Aur |the spectrum is M3 [00806].
AH    Aur |Min II 10.70. P var.
AK    Aur |VB B (A = BD +31deg 1370, 8.3m; B 82", 26deg). B - V:
AK    Aur |+0.18.
AM    Aur |Min II 11.0. P var: Min I = 2417617.2 + 13.6182d*E
AM    Aur |(JD2413500 - 19500) [00608]; since JD2425400 - see Table.
AN    Aur |B - V: +1.06,  +1.48. [A/H] =  -0.2.
AO    Aur |B - V: +0.86,  +1.27.
AP    Aur |Min II 11.2. P var: Min I = 2423080.505 + 0.5692965d*E
AP    Aur |(JD2423080 - 35000). Since JD2435000 - see Table.
AQ    Aur |Light curve shape var?
AR    Aur |Min II 6.70. Min II - Min I = 0.50004P. P var: Min I =
AR    Aur |2427887.7217 + 4.13467d*E (JD2427800 - 29500) [04999].
AR    Aur |Since JD2438400 - elements in the Table with an additional
AR    Aur |nonlinear term: -2.2d*10**(-8)*E**2.
AZ    Aur |Close companion 16.3m B.
BC    Aur |Min II 11.7.
BF    Aur |Min II 9.49. P var. Min I = 2434455.3872 +
BF    Aur |1.583217d*E (JD2411760 - 34455) [05038]. Since JD2434455
BF    Aur |- see Table. The two sets of observations are equally well
BF    Aur |represented by the formula: Min I =
BF    Aur |2440628.3643 + 1.5832212d*E + 1.7d*10**(-10)*E**2 [08160].
BH    Aur |P var. Max = 2437352.461 + 0.45608821d*E (JD2417260 -
BH    Aur |42750) [07806]. Since JD2442750 - see Table.
BK    Aur |B - V: +0.86,  +1.26.
CI    Aur |Depth of Min II 0.05m. P var. Min I =
CI    Aur |2439414.573 + 1.869984d*E + 0.020d*10**(-8)*E**2
CI    Aur |(JD2425560 - 42045). Elements given in the Table represent
CI    Aur |observations in the interval JD2439052 - 40654.
CL    Aur |Min II 12.3; Min II - Min I = 0.45P; DII = 0.13P. P var?
CL    Aur |Min I = 2432967.262 + 1.2443666d*E (JD2416900 - 32967)
CL    Aur |[00608]. Since JD2432967 - see Table.
CO    Aur |The first overtone period is
CO    Aur |given in the Table; the second overtone P = 1.4255d.
CQ    Aur |B - V: + 0.86,  + 1.07; Min II 9.14:; Min II - Min I =
CQ    Aur |0.52P:; D = 0.096P. P var. Nonlinear term:
CQ    Aur | +3.78d*10**(-7)*E**2.
CY    Aur |[A/H] =  -0.3.
DV    Aur |P var. Max = 2426015 + 198.0d*E (JD2426014 - 27400) [00332].
DV    Aur |Since JD2439940 - see Table.
EI    Aur |Min II 15.0.
EM    Aur |Min II 11.7.
EO    Aur |Min II 7.89.
EP    Aur |Min II 10.9. P var?
ER    Aur |[A/H] =  - 1.1. P var? Max = 2432951.54 + 15.69073d*E
ER    Aur |(1949 - 1950) [01059]. In the interval JD2443428 - 874 -
ER    Aur |see Table.
EW    Aur |[A/H] =  - 0.6.
FF    Aur |[A/H] =  - 0.3.
FN    Aur |Min II 12.3. P var?
FP    Aur |d = 0.080P.
FR    Aur |Min II 13.0.
FZ    Aur |d = 0.40d.
GI    Aur |Min II 11.7.
GK    Aur |Min II 14.0; Min II - Min I = 0.62P.
GO    Aur |P var. Max = 2426071 + 292.1d*E (JD2425505 -
GO    Aur |31325); Max = 2432205 + 301.2d*E (JD2432805 -
GO    Aur |36120) [03211]. Since JD2436990 - see Table.
GY    Aur |Min II 13.3.
HL    Aur |Min II 11.0.
HN    Aur |In the cluster NGC 1664.
HN    Aur |Light variations with P2 = 1400d: are
HN    Aur |superimposed by variations with P1 = 165d:.
HP    Aur |Min II 11.28; Min II - Min I = 0.502P. P var. Min I =
HP    Aur |2427445.400 + 1.4228180d*E (JD2427445 - 42683); since
HP    Aur |JD2442712 - see Table.
HR    Aur |Epoch of Min is given.
HS    Aur |Min II 11.2. The value of period given in [02619] must be
HS    Aur |doubled as the system consists of two equal components
HS    Aur |[08164].
HU    Aur |Min II 12.4.
HW    Aur |Min II 12.6.
HZ    Aur |Sometimes short period variations of Vr with the amplitude
HZ    Aur |3 km/s and of brightness in U with the amplitude 0.02m are
HZ    Aur |also observed. Max Vr = 2439454.900 + 0.073502d*E
HZ    Aur |[05259]. P (DeltaU) = 0.07396d [04818].
II    Aur |Min II 15.0:.
IM    Aur |Min II 8.05:.
IQ    Aur |Epoch of Min is given.
IS    Aur |VB. The range of combined brightness variation is given.
IS    Aur |It is not known which of the components varies.
IU    Aur |P var. There is an additional periodic term in the elements:
IU    Aur |-0.00627d*sin (2.221deg*E + 15deg). The ratio of Min II
IU    Aur |depth to Min I depth is 0.78. There is secular deepening
IU    Aur |of both minima. The depth of Min I increases by 0.016m per
IU    Aur |year. The range of light variation in the Table is given
IU    Aur |for 1979.0 (Min II 8.69). Orbital inclination is increasing
IU    Aur |by 0.5deg per year [05181] due to orbital precession caused
IU    Aur |by a third body. Spectrum description [08166].
KO    Aur |Min II 11.2.
KR    Aur |<B - V> =  +0.10, <U - B> =  -0.95. SB (P = 0.1628d [09045]).
KR    Aur |Spectrum description [08169,08170]. Wide hydrogen emission
KR    Aur |lines. Long maxima and minima lasting for years are
KR    Aur |superimposed by rapid light variations by 1 - 2m in
KR    Aur |several days or fortnights and by 0.5m in dozens of
KR    Aur |seconds [08168,08170]. The source of soft X-rays [05191].
KS    Aur |VB A (12.5m, 5", 94deg).
KV    Aur |Flat waves with a cycle about 750d are sometimes
KV    Aur |superimposed by comparatively rapid fluctuations.
KW    Aur |VB A (B 11.0m, 11.1", 352deg, 1909; C 7.99m, 14.5",
KW    Aur |226deg, 1923); SB1 (P = 3.788568d). Mean light level
KW    Aur |varies synchronously with orbital motion. Besides main
KW    Aur |pulsational period there are two more periods of nonradial
KW    Aur |pulsation: P1 = 0.096533d, P2 = 0.088243d.
KX    Aur |In the IC 405 nebula.
KY    Aur |In the IC 405 nebula.
LY    Aur |VB A (B 9.1m, 0.6", 249deg, 1958). Min II 7.26; d = 0.017P.
MR    Aur |Min II 15.5.
MT    Aur |d = 0.02P.
NP    Aur |P var. Since JD2437720 - see Table.
NU    Aur |Blazhko effect. Pi = 179d:.
NV    Aur |OH, SiO, H2O maser.
NW    Aur |In the region of the NGC 1893. Min II 14.7.
NW    Aur |According to [07160] no minimum was recorded during
NW    Aur |visual observations covering twice all phases.
NX    Aur |In the cluster NGC 1893.
OP    Aur |In the cluster Stock 8.
OX    Aur |VB A (B 10.0m, 22.4", 224deg). P1 = 0.115442d.
OX    Aur |Mean brightness probably varies.
PR    Aur |The chart in [07806] is wrong.
PY    Aur |Possibly a cepheid.
QR    Aur |Epoch of Min is given.
QY    Aur |SB.
V0348 Aur |VB A (B 13.43m, 24", 44deg).
V0353 Aur |During several decades the star brightened by 0.06m in a
V0353 Aur |year. Possibly a planetary nebula in the process of
V0353 Aur |formation.
V0358 Aur |In the region of the cluster NGC 2099.
V0411 Aur |The HD catalogue identifies HD 32447 with BD+30 775, wich
V0411 Aur |is V0411 Aur. In the HDE Atlas V0411 Aur = HD 282867, and
V0411 Aur |HD 32447 is a different star.
V0431 Aur |P = 16.86d detected in HIPPARCOS data.
V0433 Aur |SB?
V0527 Aur |Also might be a low-amplitude Cepheid.
bet   Aur |VB A (B 14.1m, 13", 174deg). Min II 1.98.
eps   Aur |VB A (B 14.0m, 21", 224deg). d = 0.037P.
eps   Aur |Survey of the physical properties of the system [02041,
eps   Aur |02042, 03070, 03216, 03217, 08174]. The spectrum probably
eps   Aur |varies even outside eclipses. The eclipses are probably
eps   Aur |due to a disk of gas and dust surrounding the hot
eps   Aur |companion. The brightness has physical fluctuations
eps   Aur |with the amplitude up to 0.24m and the cycle about 110d
eps   Aur |[02040] which hinder revealing the possible Min II.
eps   Aur |Similar cycle was discovered also in the fluctuations
eps   Aur |of Vr.
zet   Aur |Range of light variation strongly depends on lambda:
zet   Aur |4.98 - 5.53 B, 5.36 - 7.33 U. d = 0.039P var:
zet   Aur |37.58d <= d <= 38.07d [05486]. Light fluctuations of
zet   Aur |K star by 0.05m [05539].
tet   Aur |VB A (B 7.5m, 2", 8, 331deg, 1924).
tet   Aur |According to [04034] the period of magnetic field variation
tet   Aur |is 3.618d.
U     Boo |Delta(m) var (from 0.9m to 2.4m).
V     Boo |P var. Amplitude strongly varies.
W     Boo |According to [06994], P = 30d +-.
Z     Boo |H2O maser.
RS    Boo |Delta(S) = 2. P var. Before JD2435000 Max =
RS    Boo |2418115.5867 + 0.37733691d*E; since JD2435000 - see
RS    Boo |Table. Changes of the height of maxima: Max (minimal
RS    Boo |height) = JD2442500 + 533d*E; a shorter cycle of changes
RS    Boo |is possible: P ~ 58 - 62d [04832].
RU    Boo |B - V: +0.09, +0.44.
RX    Boo |H2O, SiO, OH maser.
SS    Boo |Depth of Min II 0.1m.
ST    Boo |P var. Max = 2439236.032 + 0.6222968d*E (1966 - 1974).
ST    Boo |Mean elements 1911 - 1974 - see Table. Blazhko effect: Min
ST    Boo |(O - C) = 2442203 + 284d*n. Delta(S) = 11.
SU    Boo |D = 0.032P. Min II 12.04. P var.
SV    Boo |B - V: +0.17,  +0.44. P var?
SW    Boo |B - V: +0.09,  +0.39. P var. Before JD2426500
SW    Boo |Max = 2421840.295 + 0.5134948d*E [02008,02011]. Since
SW    Boo |1960 - see Table. Secondary oscillation: Max (height of
SW    Boo |Max) = 2441037.33 + 12.997d*E. According to [04833], the
SW    Boo |magnitude in Max varies between 10.5 and 11.6 V.
SZ    Boo |P var?
TU    Boo |Min II 12.4.
TV    Boo |B - V: +0.10,  +0.22. [Fe/H] = -2.42.
TV    Boo |Blazhko effect, Pi = 16.14d [07116].
TW    Boo |B - V: +0.11,  +0.40. Delta(S) = 12. P var. Before
TW    Boo |JD2426890 Max = 2420340.551 + 0.53227557d*E;
TW    Boo |since JD2426890 - see Table.
TY    Boo |Min II 11.35.P var.
TZ    Boo |Min II 10.82 (var). dII = 0.09P. P var. Depths of minima
TZ    Boo |vary from 10.8 to 11.0 V with P ~3.5 yrs; sometimes Min II
TZ    Boo |is deeper than Min I. Some other parameters of the shape
TZ    Boo |of light curve are also variable. In ~1960 the period
TZ    Boo |changed abruptly; other period variations were also noted.
UU    Boo |B - V: +0.03,  +0.44. P var. Period change ~JD2432700
UU    Boo |[03230]. Earlier Max = 2424967.310 + 0.45690626d*E [03229].
UW    Boo |Min II 10.5.
UX    Boo |According to [02136], Delta(m) ~0.5m pg, EW?
UY    Boo |Delta(S) = 12.6. P, Delta(m) var. Before JD2425500
UY    Boo |Max = 2411459.819 + 0.6508552d*E; Max =
UY    Boo |2425688.836 + 0.6507849d*E (JD2425500 - 28670) [01702];
UY    Boo |Max = 2432306.759 + 0.650799d*E (JD2428670 - 32300)
UY    Boo |[02431]. Since JD2435900 - see Table.
VW    Boo |Min II 10.93. P var. Nonlinear term:
VW    Boo |-0.084d*10**(-9)*(E - 7500)**2.
WY    Boo |Possibly P = 90d.
XY    Boo |Min II 10.61. P var.
YZ    Boo |Delta(S) = 0. Delta(m) var, the shape of the light curve
YZ    Boo |varies [08186].
ZZ    Boo |Min II 7.44. Possible radio source.
AC    Boo |Min II 10.55. P var? Depth of minima and level of maxima
AC    Boo |are variable.
AD    Boo |Min II 9.9.
AE    Boo |P var. (k - b)2 = 0.01.
AG    Boo |Blazhko effect is possible.
AK    Boo |Min II 16.3.
AO    Boo |P var. Mean period is given.
AR    Boo |Min II 14.5. P var.
AS    Boo |Blazhko effect is possible.
BD    Boo |Blazhko effect is possible.
BE    Boo |Scatter in the light curve near max light;
BE    Boo |P var? [05264]. The value of the period in the
BE    Boo |Table may be spurious.
BG    Boo |Min II 14.3.
BI    Boo |In the region of the globular cluster NGC 5466.
BK    Boo |Min II 15.3.
BL    Boo |V 19 (NGC 5466). B - V: +0.12,  +0.25. [Fe/H] = -1.35.
BL    Boo |"Anomalous cepheid". Radial velocity cluster member.
BN    Boo |In the region of the cluster NGC 5466.
BO    Boo |The shape of the light curve varies: magnitude in
BO    Boo |Max - from 14.5 to 15.0.
BP    Boo |5.51 V.
BR    Boo |The mean light curve shows scatter which may evidence for
BR    Boo |the necessity to improve the period.
BU    Boo |P var. Mean period is given. AO Boo. The mean light curve
BU    Boo |could not be obtained.
BW    Boo |Min II 7.17. Min II - Min I = 0.450P. DII = 0.06P. SB1.
BX    Boo |VB A (B 10.6m, 36", 156deg). P var. According to other
BX    Boo |sources: Min = 244076730 + 0.741285d*E [07955];
BX    Boo |Min = 2440767.26 + 0.6080722d*E [05054].
CC    Boo |The star is not red.
CD    Boo |The star is not red.
CK    Boo |Min II 9.23.
CP    Boo |P > 0.125d.
EL    Boo |Type E: is also possible.
gam   Boo |VB A (B 12.5m, 33", 111deg, 1925). Delta(m) var. Radial
gam   Boo |velocity varies with P = 0.25d +-0.02d [04914].
kap 2 Boo |ADS 9173 A (B = kappa1 Boo, 6.69m, SB, F2V, 13",236deg).
kap 2 Boo |According to [07015], P = 0.0668d.
kap 2 Boo |Beat period ~16d [06086,07015].
ksi   Boo |ADS 9413 AB (4.7m, G8V; 6.6m, K4V; A = 4.884", P = 149.95a).
ksi   Boo |LiI lambda 6708 line is present in the G8V spectrum. Both
ksi   Boo |spectra show manifestations of chromospheric activity,
ksi   Boo |emissions of H and K Ca II. Soft X-ray source. Probably it
ksi   Boo |is component A that is variable, though variability of H
ksi   Boo |and K CaII emission with the cycle 10 - 11 years
ksi   Boo |is observed for component B.
i     Boo |ADS 9494 B (A 5.1m, G0; a = 3.8", e = 0.43, P =
i     Boo |225a). Min II 6.29. P var. Min = 2434132.517 +
i     Boo |0.267812271d*E + 0.115242d*10**(-9)*E**2 (1916 -
i     Boo |1958) [03239]; Min = 2438513.4166 + 0.2678143d*E
i     Boo |(1947 - 1967) [08191]; since 1968 - see Table. Detailed
i     Boo |studies of period changes [05222,07352,07353,08181]. Sudden
i     Boo |period changes at JD2423800, 29300, 32300, 35150 are
i     Boo |possible. The shape of the light curve and the depth of
i     Boo |Min II are also variable. According to [02020], it is also
i     Boo |possible that ADS 9494 A is variable, with the amplitude
i     Boo |up to 0.09m.
S     Cae |<B - V> =  +0.33. P < 1d.
X     Cae |(k - b)2 = 0.22.
RX    Cae |Variability type and spectral type (F3/F5II) do not agree.
R     Cam |S2/5:e. P var.
T     Cam |S5/5e.
U     Cam |Interfering P1 = 435.45d, P2 = 223.17d; P3 = 3000d [01053].
V     Cam |H2O, SiO maser.
Y     Cam |EA/SD. SB1. Min II 10.60. P var. Min =
Y     Cam |2424434.5071 + 3.3054975d*E + 0.1215d*
Y     Cam |sin (0.0543deg*E + 186.8deg) (JD2411400 - 33300) [00978];
Y     Cam |Min = 2437375.4923 + 3.3055069d*E + 5.3d*10**(-8)*E**2
Y     Cam |(JD2437375 - 41000) [07166]; since JD2440000 - see Table.
Y     Cam |The primary component is a DSCTC variable [07166] with
Y     Cam |A <= 0.05m B. According to [04192], the pulsational period
Y     Cam |is possibly synchronized with the orbital motion and
Y     Cam |remains practically constant (0.066458d) during a long time
Y     Cam |interval.
Z     Cam |SB2. Lower conjunction of the G component
Z     Cam |T = 2438470.841 + 0.289840d*E [05365]. Outside outbursts
Z     Cam |the light curve is modulated with spectroscopic elements
Z     Cam |and has a shoulder at the phase 0.88P and a broad, shallow
Z     Cam |dip at the phase 0.15P. Outside maxima flickering up to
Z     Cam |0.5m with P ~ 16s - 18s is observed. During maxima
Z     Cam |brightness fluctuations are small [05365,04193].
RS    Cam |Mean brightness varies.
RU    Cam |[A/H] =  +0.9:. P var. Min = 2417610.1 + 22.187d*E (1908 -
RU    Cam |1917), Min = 2421315.3 + 22.121d*E (1917 - 1922),
RU    Cam |Min = 2423195.6 + 22.217d*E (1922 - 1931), Min =
RU    Cam |2426350.4 + 22.138d*E (1931 - 1951), Min =
RU    Cam |2433700.2  + 22.162d*E (1951 - 1961), Min =
RU    Cam |2437356.9 + 22.055d*E (1961 - 1965) [03243].
RU    Cam |Unusual variable. The shape of the light curve varies.
RU    Cam |Before 1964 broad maxima and sharp minima were observed;
RU    Cam |Delta(m) varied by the factor  of 2, with a possible cycle
RU    Cam |5.1a [03241]. After 1964 - 1966 Delta(m) decreased abruptly
RU    Cam |(to 0.4m - 0.1m and smaller), the light curve became
RU    Cam |symmetric; the mean light varies in the range of 0.3m B.
RU    Cam |The period varies irregularly in the interval
RU    Cam |19.4d - 23.5d. Groups of oscillations are observed to
RU    Cam |replace  one another, with phase shifts up to 0.5p [04206].
RU    Cam |Unusual spectrum with intense CN and weak C2 bands.
RW    Cam |[A/H] =  +0.4. P var?
RX    Cam |B - V: +1.05,  +1.48. [A/H] = 0.
RY    Cam |Possibly P2 = 150.8d.
SS    Cam |d = 0.06P. Min II 10.35:. P var; nonlinear term:
SS    Cam |+2.04d*10**(-9)*E**2.
SV    Cam |Depth of Min II 0.15m: pg. P var. A cycle of 50a may be
SV    Cam |present in period changes. The elements in the Table are
SV    Cam |valid since 1967.5.
SW    Cam |P var. Before JD2437600 Max = 2434448 + 254.2d*E. Since
SW    Cam |JD2440000 - see Table.
SZ    Cam |Member of the open cluster NGC 1502. ADS 2984 B (A = NSV
SZ    Cam |1458 7.1m V; B 18", 304deg). Min II 7.24, D II = 0.17P.
SZ    Cam |P var. Since 1970 - see Table; earlier
SZ    Cam |Min I = 2427533.5191 + 2.6984166d*E [02071].
TU    Cam |Min II 5.22.
TV    Cam |[A/H] = -0.2.
TX    Cam |SiO maser.
UY    Cam |Delta(m) var (0.2m - 0.5m V) [03528].
UZ    Cam |P var? Before JD2428700 Max = 2427992 + 231.0d*E [00114];
UZ    Cam |since JD2440000 - see Table.
WW    Cam |d = 0.013d. Min II 11.1.
XX    Cam |During 1898 - 1980 a single symmetric Min JD2429632 was
XX    Cam |observed which lasted for 94d. Brightness fluctuations up
XX    Cam |to 0.2m during several dozens of minutes  [04271]. Hydrogen
XX    Cam |deficiency and carbon excess in the spectrum. Some authors
XX    Cam |express doubt about the star's being an RCB variable; in
XX    Cam |particular, they note the lack of IR excess [05423,05430].
AB    Cam |[A/H] = -0.1.
AD    Cam |[A/H] = -1.0.
AE    Cam |Min II 15.8.
AH    Cam |VB A (B 7"). P var. Max = 2433897.519 +
AH    Cam |0.3687404d*E (JD2427000 - 33897) [02305]. Since
AH    Cam |JD2438000 - see Table. Magnitude in Max varies with a
AH    Cam |possible cycle Pi = 46 P [03506].
AK    Cam |P var. Min = 2426393.180 + 2.226780d*E (JD2426390 - 36610)
AK    Cam |[02594]; since JD2436000 - see Table.
AS    Cam |d = 0.009P. Min II 8.97, DII = 0.06P, Min II - Min I =
AS    Cam |0.437P.
AT    Cam |Min II 10.6.
AU    Cam |Very red.
AV    Cam |d = 0.04P.
AW    Cam |Min II 8.36.
AX    Cam |Detailed spectral studies [07191], [07192].
AY    Cam |Min II 10.23, DII = 0.12P, dII = 0.02P. According to
AY    Cam |[03260], the spectrum is A5.
AZ    Cam |Min II 10.8.
BI    Cam |Delta(m) = 0.9m pg.
BK    Cam |During 1912 - 1932 periodic (P ~4.4a) spectral changes
BK    Cam |were observed which came to an end by 1937 [04282].
BM    Cam |SB1 (P = 80.174469d; e = 0.35). Epoch of Min light is given.
CZ    Cam |P = 267.79d, semiregular behavior unusual for B5 stars.
R     Cnc |SiO maser.
S     Cnc |In the field of Praesere (NGC 2632) cluster. d = 0.015P.
S     Cnc |Min II 8.39. P var.
U     Cnc |VB A (B 3"). In the field of Praesepe (NGC 2632) cluster.
V     Cnc |S0.5/6e. ADS 6763 A (B 13.5m, 10", 270deg).
RS    Cnc |P2 = 1700d. Tc lines are present in the spectrum.
RT    Cnc |P2 ~600d.
RU    Cnc |d = 0.035P. Min II 10.21:, DII <= 0.07P.
RW    Cnc |P var. Since JD2437000 - see Table. According to [02088],
RW    Cnc |Max = 2421339.380 + 0.5471932d*E +
RW    Cnc |0.57d*10**(-9)*(E - 5800)**2 + 0.028d*cos0.0215deg*
RW    Cnc |(E + 2260) + f(psi, hi); here the last term is the sum of
RW    Cnc |two short period oscillations and is given in graphical
RW    Cnc |form, since the main period (0.547d) varies with
RW    Cnc |Pi1 = 29.9d and Pi2 = 91.1d. Magnitude in Max varies from
RW    Cnc |10.7m to 11.8m, in Min from 12.3m to 12.6m.
RY    Cnc |In the region of the open cluster NGC 2632 (Praesepe),
RY    Cnc |non-member. B - V: +0.58, +1.05. P var. Before JD2436000
RY    Cnc |Min = 2429334.445 + 1.0929500d*E; since
RY    Cnc |JD2436000 - see Table.
RZ    Cnc |Min II 9.21. d = 0.015P:. Ellipsoidal components.
SS    Cnc |Delta(S) = 1.2. P var?
SV    Cnc |B - V: +0.10, +0.52.
SY    Cnc |Flickering with P ~20s - 34s [05959]. Spectral investigation
SY    Cnc |[04286].
TT    Cnc |(k - b)2 = 0.11. P var. Before JD2430700
TT    Cnc |Max = JD2425647.452 + 0.5634445d*E [03506].
TT    Cnc |Since JD2439800 - see Table. Blazhko effect, Pi = 89d
TT    Cnc |[05271].
TW    Cnc |d = 0.014P. Depth of Min II 0.1m pg.
TX    Cnc |Member of the open cluster Praesepe (NGC 2632). Min II
TX    Cnc |10.32.
TY    Cnc |d = 0.013P. P var.
UU    Cnc |Min II 9.2, JD (Min II) 2435608.5. SB1. The light curve is
UU    Cnc |unstable. Spectral studies [01881], [03149], [04289].
UV    Cnc |In the region of the Praesepe (NGC 2632) cluster.
UZ    Cnc |Min II 11.4.
VY    Cnc |Min II 12.3:.
VZ    Cnc |(k - b)2 = 0.32. Beat phenomenon for two oscillations is
VZ    Cnc |observed. According to [02125], for the middle of
VZ    Cnc |the ascending branch T (<m>)  = 2433631.84615 +
VZ    Cnc |0.17836376d*E + 0.00193d*sin(2*pi*psi(<m>) -
VZ    Cnc |0.00371d*cos*2*pi*psi(<m>); here the phase of the beat
VZ    Cnc |period psi(<m>) is computed with the elements T(<m>) =
VZ    Cnc |Spectral investigation [02126].
WW    Cnc |According to [07531], the period does not vary since 1933.
WW    Cnc |A number of minima by
WW    Cnc |BBSAG contradict the tabulated elements.
WX    Cnc |Min II 10.7.
WY    Cnc |VB A (B 12.8m,  -20", 0deg). Min II 9.60.
XX    Cnc |In the region of the Praesepe (NGC 2632) cluster.
XZ    Cnc |Min II 10.2.
YY    Cnc |According to [03263], the star is probably an irregular
YY    Cnc |variable.
YZ    Cnc |Oscillations with P = 133.2m are observed in maximum light
YZ    Cnc |[06249].
ZZ    Cnc |d = 0.02P:.
AC    Cnc |Min II 14.7. <Max> = 14.5.
AC    Cnc |The brightness outsibe eclipses varies in the range 13.8 -
AC    Cnc |15.2B. 3 deep minima contradict the tabulated
AC    Cnc |elements [04460]. The identification with the X-ray
AC    Cnc |source H 0857+13 is not excluded.
AD    Cnc |Min II 13.4.
AH    Cnc |Member of the open cluster M 67 (NGC 2682). Min II 13.68.
AH    Cnc |Nonlinear term: +1.56d*10**(-10)*E**2.
AH    Cnc |Cyclic period variations (with different cycles) are also
AH    Cnc |possible [04475].
AO    Cnc |Min II 13.4.
AP    Cnc |P var?
AU    Cnc |Possible member of the cluster praesepe (NGC 2632).
AV    Cnc |Possible member of the cluster Praesepe (NGC 2632).
AW    Cnc |Possible member of the cluster Praesepe (NGC 2632).
AX    Cnc |Possible member of the cluster Praesepe (NGC 2632).
AY    Cnc |Possible member of the cluster Praesepe (NGC 2632).
AZ    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BB    Cnc |Delta(mu) > 6.0. Possible member of the cluster
BB    Cnc |Praesepe (NGC 2632).
BC    Cnc |Delta(mu) > 4.0. Possible member of the cluster
BC    Cnc |Praesepe (NGC 2632).
BD    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BE    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BG    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BH    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BI    Cnc |The elements were determined by Winzer. Epoch of Max
BI    Cnc |in U band is given.
BK    Cnc |Possible member of the cluster Praesepe (NGC 2632).
BM    Cnc |SB (P = 585.4154d [06568]). The elements in the Table
BM    Cnc |represent the moments of maximal (B - V).
BN    Cnc |Member of the cluster Praesepe (NGC 2632).
BQ    Cnc |SB.Member of the cluster Praesepe (NGC 2632).
BR    Cnc |VB A (B 14.2m, 30", 268deg). Member of the cluster
BR    Cnc |Praesepe (NGC 2632).
BS    Cnc |Member of the cluster Praesepe (NGC 2632).
BT    Cnc |Member of the cluster Praesepe (NGC 2632).
BT    Cnc |Oscillations with other periods are superimposed.
BU    Cnc |Member of the cluster Praesepe (NGC 2632). According to
BU    Cnc |[04483], P = 0.071d is not confirmed; during different
BU    Cnc |nights P = 0.0534d, P = 0.059d and several other
BU    Cnc |periodicities were observed.
BV    Cnc |Member of the cluster Praesepe (NGC 2632).
BW    Cnc |Member of the cluster Praesepe (NGC 2632).
BX    Cnc |Member of the cluster Praesepe (NGC 2632).
BY    Cnc |Member of the cluster Praesepe (NGC 2632).
BZ    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CC    Cnc |Cycle <= 90d.
CD    Cnc |Possible member of the cluster Praesepe (NGC 2632).
CE    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CF    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CG    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CH    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CI    Cnc |Possible member of the cluster Praesepe (NGC 2632).
CK    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CL    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CM    Cnc |Possible member of the cluster Praesepe (NGC 2632).
CN    Cnc |Possible member of the cluster Praesepe (NGC 2632).
CO    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CP    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CR    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CS    Cnc |In the region of the Praesepe (NGC 2632) cluster.
CU    Cnc |G 9-8 = G 40-25. VB A (B = CV Cnc, 13", 347deg),
CU    Cnc |common mu. In the region of Praesepe (NGC 2632) cluster,
CU    Cnc |non-member.
CV    Cnc |G 40-26. VB B (A = CU Cnc).
CY    Cnc |Member of the cluster Praesepe (NGC 2632).
CZ    Cnc |Equinox in [08354] must be 2000.0.
DD    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DF    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DF    Cnc |Posibly non-member.
DG    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DG    Cnc |Possibly non-member.
DH    Cnc |Possible member of the cluster Praesepe (NGC 2632).
DI    Cnc |Possible member of the cluster Praesepe (NGC 2632).
DL    Cnc |VB. In the region of the Praesepe (NGC 2632) cluster.
DM    Cnc |Possible member of the cluster Praesepe (NGC 2632).
DN    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DO    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DP    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DQ    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DQ    Cnc |Possibly non-member.
DR    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DS    Cnc |In the regiom of the Praesepe (NGC 2632) cluster.
DS    Cnc |Possibly non-member.
DT    Cnc |In the region of the Praesepe (NGC 2632) cluster.
DU    Cnc |In the region of the Praesepe (NGC 2632) cluster.
FV    Cnc |The type is doubtful.
kap   Cnc |SB (P = 6.39316d). In [04487] the light variability was not
kap   Cnc |confirmed.
R     CVn |P var. Max = 2411768 + 325.4d*E (JD2411730 - 26430) [01701];
R     CVn |Max = 2432074 + 332.8d*E
R     CVn |(JD2426750 - 32100); since JD2432100 - see Table.
T     CVn |SRA? Delta(m) strongly varies.
U     CVn |OH, H2O emission.
V     CVn |H2O, SiO maser.
W     CVn |B - V: +0.15, +0.42. P var.
W     CVn |Nonlinear term: -368*10**(-13)*E**2. Delta(S) = 7.
Y     CVn |P2 = 2000d.
Z     CVn |B - V: +0.20, +0.33. P var. Max = 2413000.262 +
Z     CVn |0.6538236d*E (JD2413000 - 23170); Max =
Z     CVn |2423860.355 + 0.6539052d*E (JD2423860 -
Z     CVn |31800) [01702]; Max = 2432943.645 + 0.653824d*E
Z     CVn |(JD2431800 - 40200) [06457]. Since JD2438900 - see Table.
Z     CVn |Blazhko effect: Min. ampl. = 2439176.12 + 22.75d*E [03267].
Z     CVn |Amplitude varies by 0.5m B, extremal periodic deviations
Z     CVn |of the epoch of Max from linear elements are  +-0.02d.
Z     CVn |Delta(S) = 8.
RR    CVn |B - V: +0.09, +0.45. [Fe/H] = -1.33.
RR    CVn |The light curve shape and Delta(m) var.
RS    CVn |Min II 8.19; Min II - Min I = 0.506P; d = 0.033P.
RS    CVn |P var. Nonlinear term: -1.00d*10**(-8)*E**2. Wave-like
RS    CVn |distorsion with the amplitude from 0.09m up to 0.20m and
RS    CVn |with the period 4.7917d close to the orbital one is
RS    CVn |observed on the light curve out of eclipses [07209].
RS    CVn |The wave is migrating on phase in the direction of phase
RS    CVn |decreasing with a migration period of 9.48 years [05800].
RU    CVn |B - V: +0.10, +0.39. P var. Max = 2420227.338 +
RU    CVn |0.5732502d*E (JD2418801 - 29436) [05436]; Max =
RU    CVn |2420227.398 + 0.57324647d*E (JD2418979 -
RU    CVn |36665) [03271]; since JD2434483 - see Table.
RV    CVn |V141 (M3/NGC 5272). Not a member of the cluster.
RV    CVn |Min II 15.81.
RX    CVn |B - V: +0.17, +0.41. P var?
RZ    CVn |B - V: +0.12, +0.43. P var. Max = 2424621.489 +
RZ    CVn |0.56740036d*E (JD2424620 - 31000) [00188];
RZ    CVn |Max = 2437823.433 + 0.5674174d*E (JD2434470 -
RZ    CVn |37830); since JD2438200 - see Table.
ST    CVn |P var? Delta(S) = 4.8.
SV    CVn |P var. Max = 2427434.911 + 0.66805653d*E
SV    CVn |(JD2426000 - 32000) [00752]; since JD2439500 - see Table.
SW    CVn |P var. Max = 2431139.791 + 0.44164922d*E
SW    CVn |(JD2425640 - 32000) [00752]; since JD2436200 - see Table.
TX    CVn |SB2 (P = 70.8d) [04504].
UU    CVn |In the region of the globular cluster NGC 5466. P var.
UU    CVn |Max = 2437817.312 + 0.5409589d*E (JD2436360 - 39945);
UU    CVn |since JD2439945 - see Table.
UV    CVn |In the region of globular cluster NGC 5466, non-member.
UV    CVn |P var. Max = 2419446.156 + 0.6316090d*E (JD2419440 - 34455);
UV    CVn |since JD2434450 - see Table.
UW    CVn |In the region of the globular cluster NGC 5466.
UX    CVn |Min II 11.94. U - B: -1.05, -0.99; B - V: -0.29, -0.23.
VV    CVn |Min II 14.3:.
VW    CVn |Min II 12.4. P var. Min I = 2435923.246 + 0.8499757d*E
VW    CVn |(JD2427900 - 36000); since JD2435900 - see Table. The
VW    CVn |variable is not marked on the map. It is by 6mm to the
VW    CVn |west and 3mm to the north of the comparison star C.
VZ    CVn |Min II 9.54.
WW    CVn |Blazhko effect is possible.
WY    CVn |V 205 (M3/NGC 5272). Member of the cluster? Blazhko effect
WY    CVn |is possible.
WZ    CVn |V 206 (M3/NGC 5272). Non-member? Blazhko effect.
XX    CVn |In the region of M3 (NGC 5272) globular cluster. Member
XX    CVn |of the cluster?
YZ    CVn |d = 0.055P, depth of Min II 0.05m vis.
AA    CVn |[Fe/H] = -1.78.
AD    CVn |[Fe/H] = -1.39.
AF    CVn |[Fe/H] = -1.19.
AG    CVn |[Fe/H] = -2.01.
AH    CVn |[Fe/H] = -2.01.
AI    CVn |Radial multiperiod pulsations: P0 = 0.2085d,
AI    CVn |P1 = 0.1529d, P2 = 0.1259d, P3 = 0.1158d.
AK    CVn |[Fe/H] = -1.19.
AM    CVn |The light curve is a double wave. Min II sometimes
AM    CVn |disappears. The depth of Min I changes also. Epoch of
AM    CVn |Min I is given in the Table. P var; dP/dt = +0.012s per
AM    CVn |year. Elements for 1978 are given in the Table. The
AM    CVn |brightness fluctuates with the cycle of 115 - 120s,
AM    CVn |sometimes the periodicity with P = 26.3s is observed.
AM    CVn |Probably it is a close binary semidetached system of two
AM    CVn |white dwarfs with an accretion disk and a hot spot.
AN    CVn |[Fe/H] = -1.54.
AQ    CVn |Similar to horizontal branch stars in globular clusters.
AQ    CVn |A flare lasting 20 minutes was observed.
BF    CVn |G 123-75 = G 164-32. VB A (B = G 164-31, 13.16m,
BF    CVn |dM3.5e; 17", 225deg). Flares in the combined light of the
BF    CVn |system (Delta(U) up to 0.95m) were observed.
BG    CVn |P1 = 1186s, P2 = 780s.
BH    CVn |SB. Reflection effect Delta(m) = 0.013V.
BI    CVn |Min II 10.70. P var?
CS    CVn |HIPPARCOS data contradict the luminosity class V.
alf 2 CVn |VB A (B 5.60m, F0V, 19.6", 228deg).
alf 2 CVn |Epoch of Min is given.
R     CMa |Min II 5.78. P var [03280,06314].
R     CMa |The star shows anomalies of the light curve [03281,03282].
V     CMa |VB B (A = CPD -31deg 1311, 9.4 m; B 16", 90deg).
Z     CMa |Strong IR excess. Shell spectrum. Several lines show P Cyg
Z     CMa |profiles. The star is located in a nebula rich in details.
Z     CMa |A bright wisp of nebulosity near the star  has continuons
Z     CMa |spectrum, probably identical to that of the star [04002].
RR    CMa |Min II 13.1.
RT    CMa |Min II 11.5.
RT    CMa |P = 1.293745d is possible taking into account the epoch
RT    CMa |from [03283].
RX    CMa |d = 0.027P. Min II 11.1. P var. During JD2441700 - 43000
RX    CMa |- see Table.
RZ    CMa |P var? Since JD2435500 - see Table.
SW    CMa |Min II 9.9. Min II = JD2426709.366; Min II - Min I =
SW    CMa |0.316P.
SX    CMa |Min II 10.3.
TU    CMa |Min II 10.1.
UW    CMa |Min II 5.25. Gaseous streams, expanding gaseous envelope.
UW    CMa |Minima are asymmetric; other peculiarities of the light
UW    CMa |are observed. A number of spectral lines have P Cyg
UW    CMa |profiles.
UW    CMa |The line profiles are observed to vary with the phase of
UW    CMa |the orbital period, and also ([07227], according to Sanyal)
UW    CMa |with characteristic time <1h.
UX    CMa |Min II 12.3.
VW    CMa |Min II 9.1.
VY    CMa |ADS 6033 A (B 9.2m, 0.5", 168deg; C 11.5m, 2.7", 291deg,
VY    CMa |D 11m, 2.9", 347deg, ...). H2O, OH, SiO maser.
VY    CMa |B - V:  +2.3.
VY    CMa |In the region of the
VY    CMa |young open cluster NGC 2362. Embedded in a
VY    CMa |reflecting nebula. The companions may be details
VY    CMa |of the nebula; some of them are probably variable [02159,
VY    CMa |03287]. Surrounded by an envelope of gas and dust or a disk
VY    CMa |of 0.45" (lambda = 5 mkm) angular size. Secular decrease
VY    CMa |of brightness since 1801. Cyclic variations of brightness
VY    CMa |with Delta(m) from several tenths of a magnitude to 3m on
VY    CMa |time scale from 200d to 1900d. TiO and ScO emission bands
VY    CMa |in the spectrum. Spectroscopic studies [03287,05282,06133].
WW    CMa |RR, Max = 2428570.09 + 0.499355d*E [00613]. CEP,
WW    CMa |Max = 2428146.6 + 5.7660d*E [00514]. These systems of
WW    CMa |elements are contradicted by 94 photographic observations
WW    CMa |(Erleksova) and 12 photoelectric observations (Irwin,
WW    CMa |[03288]).
XY    CMa |d = 0.04P:.
ZZ    CMa |Min II 13.0.
AE    CMa |d = 0.02P:.
AN    CMa |d = 0.02P:.
AO    CMa |In the field of the open cluster Ruprecht 18.
AR    CMa |d = 0.025P:.
AS    CMa |d = 0.04P.
BN    CMa |Min II 14.9.
BQ    CMa |In the region of the open cluster NGC 2354.
BS    CMa |Min II 14.5.
CC    CMa |Mean brightness varies?
CE    CMa |Min II 13.3. Min II - Min I = 0.663P.
CH    CMa |Min II 12.9.
CK    CMa |Min II 15.4.
CM    CMa |Min II 13.1.
CO    CMa |Mean brightness probably varies with P ~700d.
CR    CMa |Min II 12.4.
CV    CMa |Min II 13.5. DII = 0.09P. Min II - Min I = 0.358P.
CW    CMa |Min II 8.94. SB2.
CX    CMa |Min II 10.3.
DD    CMa |Min II 11.8.
DE    CMa |Min II 13.4.
DS    CMa |VB A (B 15.8m, 10", 130deg).
DV    CMa |JD2425300 - 27500: P - see Table; since JD2428000 P ~400d.
EF    CMa |d = 0.02P.
EW    CMa |VB Delta(m) <= 0.5m, 0.102", 112.1deg, 1952.203).
EW    CMa |SB (P = 0.261975d). Brightness variations are not related
EW    CMa |to the orbital phase. Shell star (probably an extended
EW    CMa |atmosphere of one of the components and the common shell
EW    CMa |around the system). Spectral studies {4592 - 4596}.
EX    CMa |Was faint for 2 nights (October 8 and 9, 1962).
EY    CMa |P var, Delta(m) var [03960]. The main wave is superimposed
EY    CMa |by secondary ones (P = 0.2033d and 0.1690d); beat effect,
EY    CMa |Pb ~2.00d [07243].
EZ    CMa |SB. In the centre of the ring HII region S 308. Member of
EZ    CMa |the open cluster collinder 121. Epoch of Max light is
EZ    CMa |given. The companion is probably a neutron star. The shape
EZ    CMa |of the light curve, Delta(m), phases of maxima and minima
EZ    CMa |and mean light vary from one observational season to
EZ    CMa |another.
FF    CMa |Min II 7.6. Elements should be improved. Member of the
FF    CMa |open cluster Cr 132a.
FM    CMa |Min II is almost as deep as Min I [06585].
FN    CMa |VB (6.3m,  7.5m, 0.561", 115.8deg, 1978.15). Range of
FN    CMa |combined light variation is given in the Table.
FN    CMa |Associated with the nebula vB 95. According to [06135],
FN    CMa |the period considerably differs  from the tabulated value.
FQ    CMa |Min II 9.7.
FR    CMa |ADS 4978 AB (6.2m, 10.4m, 4", 23deg; C 11.62m, 56").
FS    CMa |Extended shell of gas and dust. Emissions of [FeII],
FS    CMa |[NiII], [CrII], [SII], [OI], FeII. IR excess
FS    CMa |(1.6 - 20 mkm). P Cyg profiles of Balmer lines vary in the
FS    CMa |time scale of hours. Brightness varies from night to night
FS    CMa |by 0.1m and during a night by 0.03m, sometimes in
FS    CMa |correlation with spectral changes [06636]. Spectral
FS    CMa |studies [07250,07251,07253].
FT    CMa |VB A (B 12.58m, 36", 97deg).
FU    CMa |VB A (B 14.7m, 14", 230deg, 1897; C 11.07m, 40", 225deg).
FW    CMa |VR var, P = 31.9045d [06154].
FZ    CMa |Min II 8.44. In the HII region S 295, in the association
FZ    CMa |CMa OB1.
GG    CMa |Member of the open cluster Cr 132a.
GU    CMa |ADS 5713 AB (7.5m, 8.2m, 0.6", 187deg, 1919). SB?
GU    CMa |In the HII region S 293.
GY    CMa |According to [08380], does not vary.
GZ    CMa |SB2.
HK    CMa |Epoch of Min is given.
HL    CMa |1E 0643.0-1648. SB (P ~0.217d); Lx/Lopt var (0.002 - 1).
IU    CMa |Type LBV: is also possible.
MO    CMa |The amplitude can have been overestimated (M. Grenon, private
MO    CMa |communication).
NO    CMa |Type LBV: is also possible.
bet   CMa |In 1971 - 72 the observations were described by the
bet   CMa |combination of the tabulated elements (period P1) and the
bet   CMa |following systems of elements:
bet   CMa |Max = 2441296.0705 + 0.251300d*E, (P2);
bet   CMa |Max = 2441296.032 + 0.23904d*E, (P3);
bet   CMa |Max = 2441296.065 + 0.12501d*E, (P1/2);
bet   CMa |Max = 2441296.124 + 0.12565d*E, (P2/2).
bet   CMa |Beat periods:  49.198d, 5.442d, 4.900d.
bet   CMa |Since 1908 P1 increases, P2 decreases. 12 overtone and
bet   CMa |resonance periods were found in [03454].
ksi 1 CMa |ADS 5176 A (B 14.5m, 25", 147deg; C 14.0m, 29", 303deg,
ksi 1 CMa |1897).
sig   CMa |ADS 5719 A (14.2m, 11", 153deg, 1926).
tau   CMa |SB, Porb = 154.90d.
ome   CMa |SB?
R     CMi |SC4/10e.
T     CMi |P var. Max = 2422456 + 324.2d*E (JD2416610 -
T     CMi |22800); Max = 2430896 + 311.2d*E (JD2423090 -
T     CMi |30900); since JD2430900 - see Table.
U     CMi |There is a hump on the ascending branch looking sometimes
U     CMi |as a secondary maximum. The light curve for 1904 - 1970
U     CMi |[07368].
X     CMi |P var? Delta(S) = 3.
RS    CMi |d = 0.02P:.
RX    CMi |Min II 14.6; Min II - Min I = 0.52P:.
RY    CMi |Min II 12.0:.
SX    CMi |DI <= 0.12P. Min II 13.6.
SY    CMi |P var. Max = 2425234.682 + 0.565900d*E (JD2425234 - 708);
SY    CMi |since JD2436586 - see Table.
TU    CMi |Min II 15.1.
TW    CMi |Min II 15.6.
TX    CMi |Min II 14.7.
UZ    CMi |Min II 12.1.
XZ    CMi |Min II 9.88. P var?
YY    CMi |Min II 8.88.
YZ    CMi |mu = 0.604", P = 221.4deg. Epoch of Min is given. P var;
YZ    CMi |additional term: -0.00003919514d*E*(E + 1)/2. Periodical
YZ    CMi |light variations with the amplitude 0.12m (11.26 - 11.38 V)
YZ    CMi |are superimposed by strong flares.
AG    CMi |P var. Min = 2434698.670 + 1.6645729d*E (JD2426350 -
AG    CMi |34740) [01727]. Since JD2437650 - see Table.
AH    CMi |EW?
AK    CMi |Min II 10.3; Min II - Min I = 0.55P. P var. Min I =
AK    CMi |2425352.348 + 0.56589534d*E (JD2424880 -
AK    CMi |35550) [01728]. Since JD2435600 - see Table.
AL    CMi |Observations in the interval JD2424880 - 25950 are
AL    CMi |represented by the elements: Max = 2425243.631 + 0.55050d*E.
AL    CMi |Since JD2436590  -  see Table.
AM    CMi |Min II 10.5.
AN    CMi |d = 0.02P:.
AO    CMi |d = 0.01P:. Min II 14.5.
BF    CMi |Depth of Min II 0.05m:.
BO    CMi |Several episodes of outburst-like activity.
RS    Cap |Mean brightness varies with P = 3360d.
RT    Cap |VB A (B 15m, 26", 227deg).
RU    Cap |VB A (B 13.6m, 1.6", 86deg).
RV    Cap |<P> var: Max = 2424334.6612 + 0.44775262d*E
RV    Cap |(JD2417400 - 33610) [00323]. Since JD2433850 - see Table.
RV    Cap |Light curve and period vary with the Blazhko effect
RV    Cap |period Pi = 225.5d [06464]. Semiamplitude  of deviations
RV    Cap |from linear elements is +-0.032d. 0.14P <= M - m <= 0.25P.
RV    Cap |(k - b)2 = 0.05.
RW    Cap |d = 0.020P. Min II 9.9. P var. Min I  = 2418924.594 +
RW    Cap |3.3923922d*E (JD2418920 - 24000) [06774];
RW    Cap |Min I  = 2424003.014 + 3.3923457d*E (JD2424000 -
RW    Cap |34500) [02389]; since JD2435400 - see Table.
RX    Cap |Min II 12.5.
RY    Cap |VB B (A 7.1m, F0; B 6.6", 90deg; C 12.0m, 8.5", 58deg).
TV    Cap |<P> = 67d [01331].
TW    Cap |P var. P = 28.6421871d (JD2414000 - 17600);
TW    Cap |P = 28.61700115d (JD2417600 - 24000) [01331];
TW    Cap |Max = 2426211.90 + 28.59497d*E (JD2421400 -
TW    Cap |26200) [02390]; Max = 2435664.8 + 28.5578d*E
TW    Cap |(JD2426210 - 37500) [02309]; since JD2437500 - see Table.
TW    Cap |0.14P <= M - m <= 0.40P. [Fe/H] =  -0.72.
TY    Cap |Min II 10.6. P var. Min I hel = 2432017.956 + 1.423466D*E
TY    Cap |(JD2425500 - 35000); since JD2435000 - see Table.
UW    Cap |Min II 11.5; Min II - Min I = 0.5P. P var? Min I =
UW    Cap |2434627.290 + 1.399118d*E (JD2427000 - 35000);
UW    Cap |since JD243500 - see Table.
YZ    Cap |(k - b)2 = 0.08.
AD    Cap |Outside eclipses B - V =  +1.00. P var?
AE    Cap |Mean brightness varies with P = 2300d.
BH    Cap |Type RR: is also possible.
BN    Cap |The variability may be due to the fainter (B) component.
del   Cap |VB A (B 15.8m, 69", 94deg; C 12.7m, 119", 302deg,
del   Cap |1911); mu = 0.391", P = 138.8deg. Min II 2.90.
del   Cap |The light curve shape var? [03305].
eps   Cap |VB A (B 9.52m, 68.7", 47deg).
R     Car |VB A (B 12m, 2.1", 138deg). H2O, SiO maser.
U     Car |P var. Max = 2429023.80 + 38.753d*E (JD2415000 -
U     Car |29500); since JD2429500 - see Table.
V     Car |The light curve shape var?
X     Car |Min II 8.6.
Y     Car |VB A (B 12.22m, 15"; C 12.96m, 30"). SB (P = 400 - 600d)
Y     Car |[05119]. The fundamental mode period P0 is given in the
Y     Car |Table (A = 0.58m). The first overtone period P1 = 2.55954d
Y     Car |[05119] (A = 0.28m). P1/P0 = 0.7032.
RR    Car |P var. <P> = 154d (JD2421500 - 23500); <P> = 259d
RR    Car |(JD2426400 - 30100); <P> = 154d (JD2430400 - 33100).
RR    Car |S6.5/1- .
RT    Car |In the region of the cluster Tr 15.
RY    Car |There is a close companion 14.3 pg. P var.
RY    Car |Max = 2418475 + 416d*E (JD2415140 - 18500);
RY    Car |Max = 2429901 + 417.3d*E (JD2423600 - 32900);
RY    Car |since JD2434100 - see Table.
ST    Car |Depth of Min II 0.27m.
SW    Car |Depth of Min II 0.05m.
SZ    Car |In the region of the cluster NGC 3114.
TX    Car |The light curve shape var?
TZ    Car |Mean brightness varies with P = 1183d; the amplitude of
TZ    Car |the short cycle is large in mean brightness maximum and
TZ    Car |small during its minimum.
UX    Car |In the region of the cluster IC 2581.
VV    Car |In the region of the very poor cluster N 99 [07374]
VV    Car |(10h 36.0m -58deg 56', 1950.0) embedded in a nebula.
VY    Car |VB A (B 11.07m; B 9V:, 10", 150deg). P var.
VY    Car |Nonlinear term: -0.000021d*E**2 (JD2410000 - 44200).
VY    Car |The latest observations may be represented also by linear
VY    Car |elements: Max = 2444161.16 + 18.9138d*E
VY    Car |(JD2441000 - 44200). [A/H] = 0.4.
WZ    Car |P var. Max = 2419981.099 + 23.000945d*E (JD2410000 - 20000)
WZ    Car |[00025]; Max = 2423984.12 + 23.0054d*E (JD2419800 - 25500)
WZ    Car |[00322]; Max = 2434914.86 + 23.0075d*E + 0.000025d*E**2
WZ    Car |(JD2434500 - 41200) [02309]; since JD2434500 - see also
WZ    Car |Table.
XX    Car |P var. Max = 2420769.703 + 15.723704d*E (JD2410000 - 22500)
XX    Car |[00025]; P = 15.7196d (JD2423000 - 30000) [00003]; since
XX    Car |JD2434500 - see Table; elements given in the Table contain
XX    Car |a nonlinear term: -0.0000034d*E**2.
XY    Car |[A/H] = 0.1.
XZ    Car |[A/H] = 0.2.
YZ    Car |P var. Nonlinear term: +0.0000022d*E**2. [A/H] = -0.1.
AE    Car |In the region of the cluster NGC 3532.
AF    Car |P var. Max = 2434532 + 433.7d*E (JD2420200 - 34600); since
AF    Car |JD2435000 - see Table.
AG    Car |Central star of the low-excitation planetary nebula
AG    Car |P.K.289-0.1 ejected probably during a nova-like outburst
AG    Car |of the star about 1000 years ago [07052,07113].
AS    Car |d = 0.025P.
AW    Car |d = 0.015P.
BL    Car |In the region of the cluster Tr 16.
BO    Car |VB A (B 11.05m V, B8III, 10", 41deg). In the region of
BO    Car |the cluster Tr 15. Cluster non-member.
BP    Car |P = 4.82246d?
BS    Car |In the region of the cluster IC 2602. Min II 15.3.
BZ    Car |Mean brightness possibly varies with P = 1800d.
CD    Car |In the centre of the cluster Cr 236.
CF    Car |In the region of the cluster NGC 3496.
CI    Car |In the region of the cluster NGC 3572. d = 0.021P?
CO    Car |d = 0.024P?
CV    Car |d = 0.046P. Depth of Min II 0.05m.
DE    Car |d = 0.016P?
DH    Car |VB B (A 15.2m V; B 13", 350deg). B - V = +0.90m
DH    Car |(Min brightness).
DI    Car |Besides Cepheid-like light variations with the amplitude
DI    Car |1.7m and elements Max = 2438553.70 + 29.210d*E
DI    Car |(JD2438465 - 40300) [05324] large weakenings of brightness
DI    Car |are observed [04678]. At Max B - V = +1.34.
DK    Car |d = 0.07P.
DM    Car |d = 0.040P.
DP    Car |d = 0.034P. Min II 13.1.
DS    Car |d = 0.03P.
DU    Car |In the region of the cluster IC 2602.
DW    Car |In the region of the cluster Cr 228. Min II 10.3.
EF    Car |d = 0.04P.
EG    Car |In the region of the cluster NGC 3532.
EH    Car |VB A (B 15", 320deg).
EK    Car |In the region of the cluster NGC 3532.
EM    Car |Min II 8.9.
EN    Car |In the region of the cluster Tr 18.
EQ    Car |d = 0.030P. Min II 13.7.
ER    Car |In the region of the cluster NGC 3532.
ES    Car |In the region of the cluster NGC 3572.
EZ    Car |Min II 9.8.
FI    Car |P var. Max = 2425446.81 + 13.4542d*E (JD2423790 - 35300)
FI    Car |[00046,02309]. Since JD2435300 - see Table.
FK    Car |VB.
FO    Car |VB A (B 14m, 7", 90deg). P var. Max = 2434922.531 +
FO    Car |10.3559d*E (JD2423700 - 35300) [06006]; since JD2436000
FO    Car |- see Table. B - V: +1.13, +1.43.
FP    Car |d = 0.01P:.
FQ    Car |In the region of the cluster Tr 18.
FS    Car |In the region of the very poor cluster N 99 [07374] (10h
FS    Car |36.0m -58deg 56', 1950.0) embedded in a nebula. Min II
FS    Car |10.9.
FT    Car |According to [02197] spectrum C. Misidentification is
FT    Car |possible.
FV    Car |VB A (B 13m, 10", 135deg). P var. There are two additional
FV    Car |terms in the elements given in the Table:
FV    Car |-0.1065d*10**(-7)*E**2 - 0.584d*10**(-11)*E**3.
FV    Car |d = 0.02P:. Min II 13.0.
GG    Car |Min II 9.5. Gas and dust envelope.
GH    Car |In the region of the cluster Tr 18.
GK    Car |In the region of the cluster Tr 19. Min II 13.2.
GL    Car |In the region of the cluster NGC 3572. Min II 10.31.
GL    Car |System with the apsidal motion; e = 0.157, omega = 99deg.
GL    Car |There are sinusoidal terms in the elements for Min I given
GL    Car |in the Table: +0.121d sin(0.094389deg*E) -
GL    Car |0.007d sin(0.188778deg*E);
GL    Car |Min II = 2424263.236 + 2.4222338d*E -
GL    Car |0.121d sin(0.094389deg*E) - 0.007d sin(0.188778deg*E).
GL    Car |DII = 0.17P.
GM    Car |In the region of the very poor cluster N 99 [07374] (10h
GM    Car |36.0m -58deg 56', 1950.0) embedded in a nebula.
GM    Car |Min II 9.22.
GN    Car |Min II 12.1.
GO    Car |VB A (B 15", 60deg).
GP    Car |Min II 12.8.
GQ    Car |Min II 13.5.
GR    Car |Min II 14.0; Min II - Min I = 0.316P; DII = 0.05P.
GV    Car |Possible member of the cluster NGC 3532. Min II 9.1.
GW    Car |Min II 9.9.
GZ    Car |Light elements for the fundamental mode oscillation with
GZ    Car |an amplitude 0.16m are given in the Table. For the first
GZ    Car |overtone oscillation with an amplitude 0.07m
GZ    Car |Max = 2440742.4 + 2.93424d*E. Epochs of maxima and
GZ    Car |amplitudes are given according to [05175].
HH    Car |VB A (B 13.0m, 5", 260deg; C 11.11m, 13", 337deg; D 12.65m,
HH    Car |15", 7deg). d = 0.02P. Min II 10.66. P var [08094].
HH    Car |Min I hel = 2430860.162 + 3.2315393d*E (JD2427590 - 35260)
HH    Car |[05292]. Possible current elements are given in the Table.
HI    Car |Min II 10.8.
HK    Car |VB A (B 12.5m, 4"). Range of combined brightness variation
HK    Car |is given.
HL    Car |d = 0.03P:.
HN    Car |Min II 12.5.
HP    Car |VB A (B 9.1m, 0.4", 178deg). Min II 9.3. Elements should
HP    Car |be corrected [08083].
HQ    Car |B - V: +0.63,  +1.04.
HR    Car |Spectrum description  [01914,06466].
HT    Car |In the region of the cluster IC 2581. Min II 14.0.
HV    Car |d = 0.026P. Min II 14.2.
HW    Car |Epoch of Min is given.
HX    Car |Min II 14.5.
IK    Car |In the region of the cluster NGC 2602.
IL    Car |Min II 14.4.
IN    Car |It is possible that the period must be doubled.
IQ    Car |In the region of the cluster NGC 3532.
IR    Car |In the region of the cluster NGC 3532. Min II 12.6.
IS    Car |Min II 14.0.
IU    Car |(k - b)2 = 0.02.
IW    Car |Mean brightness varies with the period close to 1500d, the
IW    Car |amplitude of main oscillations - from 1.3m to 0.3m.
IX    Car |In the centre of a bright nebula with the diameter 2.4'.
IZ    Car |Declination in [00085] is wrong by 3deg. Identical to
IZ    Car |V336 Car, see [06316].
KQ    Car |Min II 10.3.
KU    Car |Min II 11.6.
MP    Car |VB A (B 16m, 180deg).
MZ    Car |sf component of a close pair.
OO    Car |Min II 14.7.
OV    Car |Min II 13.5.
OY    Car |Eclipse elements:
OY    Car |Min I hel = 2443993.553241 + 0.0631209247d*E [05185];
OY    Car |D = 0.050P, d = 0.044P. The hump on the light curve is
OY    Car |observed at the phase of 0.75P. Depth of Min I varies
OY    Car |between 1.48m and 2.47m.
PT    Car |Min II 13.0:.
PX    Car |Min II 10.10.
QR    Car |Min II 10.4.
QS    Car |Min II 9.3.
QU    Car |HDE 310376 (HA 112, 173). Flickering resembles V818 Sco.
QU    Car |Variations by 0.2m in 90s were observed. No periodicity
QU    Car |was found. Emission lines He II 4686, CIV - NIII 4630 -
QU    Car |4650 and sometimes weak hydrogen absoptions (corresponding
QU    Car |to A or B type) are noticeable in the spectrum [05643].
QX    Car |Min II 7.02.
QY    Car |In the open cluster No.90 [07374].
QZ    Car |In the eta Carina nebula, possible member of the cluster
QZ    Car |Collinder 228. Min II 6.43. Two SB1 systems (A and B),
QZ    Car |B is eclipsing (A: SB1, P = 20.73d, O9.5 I,
QZ    Car |Delta(m) = 0.6m). Combined brightness is given.
V0341 Car |In the variable reflecting nebula IC 2220. In the region
V0341 Car |of the open cluster NGC 2516. IR excess.
V0343 Car |VB. SB (P = 133.92d).
V0347 Car |Deep Min II.
V0348 Car |In the open cluster IC 2581. Min II 8.9.
V0354 Car |Very red.
V0356 Car |Member of the cluster NGC 2516.
V0357 Car |SB (P = 6.74483d [04627]).
V0361 Car |In the region of the cluster NGC 3293.
V0365 Car |In the region of the cluster NGC 3532.
V0367 Car |Min II 7.54.
V0373 Car |Member of the cluster NGC 2516.
V0374 Car |Member of the cluster NGC 2516.
V0375 Car |P = 0.264d or 0.359d.
V0376 Car |VB A (B 6.83m, B 9.5V, 41", 75deg).
V0378 Car |In the open cluster NGC 3293.
V0379 Car |In the open cluster NGC 3293.
V0380 Car |In the open cluster NGC 3293.
V0381 Car |In the open cluster NGC 3293.
V0382 Car |In the region of the cluster NGC 3532.
V0385 Car |Depth of Min II 0.04m. Surrounded by a ring nebula RCW 58.
V0491 Car |Mean magnitude 9.69.
V0493 Car |SB, Porb = 3.368d.
V0498 Car |Type BE: is also possible.
V0534 Car |Flare-like activity.
eta   Car |In the emission nebula NGC 3372 in the region of the
eta   Car |cluster Tr 16. A very massive young star surrounded by an
eta   Car |expanding gas and dust shell with the diameter 2" at 2mu
eta   Car |and 6.5" at 12.2mu. Maximum brightness was observed in
eta   Car |1843. Since 1880 varies in the range 5.9 - 7.9 V. In the
eta   Car |interval JD2434000 - 41000 Max = 2434037 + 1110d*E. There
eta   Car |are emission lines of H, HeI, FeII, [FeII], etc. in the
eta   Car |spectrum. Description of the spectrum [05251,07279].
eta   Car |Soft X-ray source of variable intensity.
khi   Car |Soft X-ray source.
R     Cas |VB A (B 14.5m, 14", 273deg). SiO, OH maser;
R     Cas |sometimes H2O emission.
T     Cas |SiO maser. ZrO bands in the infrared spectral region.
U     Cas |S4.5/4e.
W     Cas |SC5/9e.
X     Cas |P var: Max = 2426650 + 432.32d*E (JD2416750 - 27060);
X     Cas |Max = 2432870 + 413.6d*E (JD2427060 - 32870);
X     Cas |Max = 2437948 + 423.0d*E (JD2432870 - 39210).
X     Cas |Current elements are given in the Table.
Y     Cas |OH, H2O emission; SiO maser.
Z     Cas |SiO maser.
RS    Cas |P var. Max = 2416942.16 + 6.29552d*E (JD2412650 - 34900)
RS    Cas |[03317]. Since JD2434900 - see Table.
RV    Cas |There are signs of Se type in the spectrum [03383].
RW    Cas |P var. Max = 2421354.22 + 14.8004d*E (JD2417000 - 30000).
RW    Cas |Since JD2430000 - see Table. [A/H] = 0.3.
RX    Cas |Unigue rapidly evolving eclipsing system. 9.12<=Min II<=9.49;
RX    Cas |Min II - Min I = 0.5070P. P var. Nonlinear term:
RX    Cas |+1.017d*10**(-5)*E**2. Observations may be represented
RX    Cas |also by three systems of elements: Min I =
RX    Cas |2416250.889 + 32.31481d*E (0 <= E <= 286,
RX    Cas |JD2416250 - 25482); Min I = 2416248.835 + 32.32145d*E
RX    Cas |(331 <= E <= 554, JD2426940 - 34155);
RX    Cas |Min I = 2416244.990 + 32.32765d*E (734 <= E <= 876,
RX    Cas |JD2439970 - 44570). Brightness of the system out of
RX    Cas |eclipses periodically varies within 8.6m - 9.0m with
RX    Cas |elements Max = 2416198 + 516.06d*E [05036]. Max - Min =
RX    Cas |233d = 0.45P [00881]. Strong emissions of H, NV, CIV,
RX    Cas |SIIV, FeIII. Powerful gaseous stream and accretion
RX    Cas |phenomena are possible.
RY    Cas |[A/H] = 0.0.
RZ    Cas |Min II 6.26. The light curve shape var; d var
RZ    Cas |(0.000P <=  d <= 0.009P). P var, variations are irregular.
RZ    Cas |Mean elements based on visual and photographic
RZ    Cas |observations: Min I = 2416886.8806 + 1.195253065d*E
RZ    Cas |(JD2416800 - 26700) [08820], Min I = 2432820.7853 +
RZ    Cas |1.1952517d*E (JD2426700 - 34000) [00938]. From
RZ    Cas |photoelectric observations: Min I = 2432115.5827 +
RZ    Cas |1.1952472d*E (JD2429870 - 30400); Min I =
RZ    Cas |2432085.7011 + 1.195259d*E (JD2432000 - 32460);
RZ    Cas |Min I = 2434349.5130 + 1.1952525d*E (JD2432450 - 34420);
RZ    Cas |Min I = 2434703.3035 + 1.195238d*E (JD2434420 - 34705);
RZ    Cas |Min I = 2435934.4087 + 1.1952499d*E (JD2434705 - 35950);
RZ    Cas |Min I = 2438829.2818 + 1.195243d*E (JD2436800 - 39100);
RZ    Cas |Min I = 2440182.3089 + 1.195259d*E (JD2439380 - 40200);
RZ    Cas |Min I = 2441333.3257 + 1.195244d*E (JD2440500 - 41350);
RZ    Cas |Min I = 2442327.7798 + 1.1952521d*E (JD2441550 - 42350);
RZ    Cas |since JD2442850 - see Table.
SU    Cas |[A/H] = -0.1.
SV    Cas |P var. Max = 2421839 + 279.3d*E (JD2417600 -
SV    Cas |21900); Max = 2430450 + 281.7d*E (JD2422500 -
SV    Cas |31900); since JD2432600 - see Table.
SX    Cas |VB A (B 11.5m, 19", 250deg, 1966). Min II 9.32. The light
SX    Cas |curve shape var. DII = 0.171P:, dI = 0.036P, dII = 0.050P.
SX    Cas |P var. Min I = 2433963.267 + 36.56727d*E (JD2418000 -
SX    Cas |37000); since JD2438700 - see Table. Strong emissions
SX    Cas |of H, NV, CIV, SIIV, FeIII. Gaseous streams and accretion
SX    Cas |phenomena.
SY    Cas |VB? P var. Max = 2417911.547 + 4.070969d*E
SY    Cas |(JD2417000 - 34000); since JD2434000 - see Table.
SZ    Cas |P var. Max = 2421261.66 + 13.6009d*E (JD2416700 - 21260);
SZ    Cas |Max = 2426650.20 + 13.6072d*E (JD2421260 - 27170) [08821];
SZ    Cas |Max = 2429727.240 + 13.61744d*E (JD2427170 - 33050);
SZ    Cas |Max = 2436810.92 + 13.62655d*E (JD2433050 - 38720);
SZ    Cas |since JD2438720 - see Table. [A/H] = -0.6.
TU    Cas |Fundamental mode period P0 is given in the Table; the
TU    Cas |corresponding amplitude is 0.69m. First-overtone period
TU    Cas |P1 = 1.51830d; the corresponding mean amplitude decreased
TU    Cas |from 0.4m to 0.25m during 67 years [05078]. P1/P0 = 0.71.
TU    Cas |M - m var (0.17P <=  M - m <= 0.35P).
TV    Cas |d = 0.01P. Min II 7.34. The light curve shape var.
TV    Cas |Period of these variations - 600d [08822]. P var. Mean
TV    Cas |elements based on visual and photographic observations:
TV    Cas |Min I = 2432827.7665 + 1.81260983d*E (JD2415650 - 32800)
TV    Cas |[01926]. From photoelectric observations Min I =
TV    Cas |2432827.7665 + 1.8126142d*E (JD2432800 - 36490);
TV    Cas |Min I = 2436483.8091 + 1.81255d*E (JD2436480 - 36980);
TV    Cas |Min I = 2438472.2386 + 1.81263d*E (JD2437000 - 38500);
TV    Cas |Min I = 2438829.3230 + 1.8126048d*E (JD2438470 - 41750);
TV    Cas |since JD2441750 - see Table.
TW    Cas |Min II 8.40.
TX    Cas |Min II 9.6.
TY    Cas |P var. Max = 2419260 + 545.0d*E (JD2419200 - 25300);
TY    Cas |Max = 2428965 + 623.8d*E (JD2427000 - 41500);
TY    Cas |since JD2441500 - see Table.
UU    Cas |Min II 10.5.
UZ    Cas |[A/H] = -0.3.
VV    Cas |P var. Max = 2422514.16 + 6.207510d*E (JD2417000 - 32500);
VV    Cas |since JD2432500 - see Table. [A/H] = -0.2.
VW    Cas |[A/H] = 0.0.
WY    Cas |In the region of the cluster NGC 7789.
WY    Cas |The spectrum of the G type star is seen in minimum light
WY    Cas |[03502]. The existence of a physical companion is possible.
WY    Cas |S6/6-e.
WZ    Cas |VB A (optical companion B 8.7m, 58", 89deg). SC7/10e.
WZ    Cas |Light variations are sometimes taking place with doubled
WZ    Cas |period.
XX    Cas |Min II 10.2.
YZ    Cas |VB A (B 11.23m, 35", 160deg). d = 0.045P. Min II 5.78.
ZZ    Cas |Min II 10.9.
AB    Cas |EA/SD. Min II 10.28. P var. Min I = 2430755.678 +
AB    Cas |1.366863d*E (JD2425400 - 33150); Min I =
AB    Cas |2433616.532 + 1.366876d*E (JD2433150 - 37000);
AB    Cas |Min I = 2440475.5216 + 1.3668783d*E (JD2437000 -
AB    Cas |41600); since JD2441600 - see Table.
AB    Cas |The A3 component is a DSCT type variable with the elements:
AB    Cas |Max hel = 2444912.1759 + 0.0582874d*E [08825]; amplitude
AB    Cas |of pulsations Delta(V) var (0.03m <= Delta(V) <= 0.09m).
AE    Cas |Min II 12.8.
AH    Cas |Min II 13.3.
AL    Cas |Min II 13.6.
AO    Cas |Min II 6.24. The light curve shape var. P var?
AQ    Cas |Min II 10.4.
AR    Cas |VB A (B 9.3m, 1.0", 336deg; C 8.2m, 75", 269deg;
AR    Cas |D 9.8m, 76", 268deg; E 11.28m, 43", 115deg; F 11.06m, 69",
AR    Cas |338deg; G 11.11m, 67", 348deg). Min II 4.86;
AR    Cas |Min II - Min I = 0.614P; DII = 0.076P; dII = 0.037P.
AS    Cas |VB A (B 15.5m, 3", 45deg).
AS    Cas |Fundamental mode period P0 is given in the Table; the
AS    Cas |corresponding amplitude is 0.59m. First-overtone period
AS    Cas |P1 = 2.2909d; amplitude of oscillations with this period
AS    Cas |is 0.13m. P1/P0 = 0.76.
AX    Cas |Min II 12.9.
AZ    Cas |B - V: +1.78, +2.20. D = 110d, d = 88d = 0.026P.
BD    Cas |B - V: +1.50, +1.61. P var. Max = 2429124.84 +
BD    Cas |3.65129d*E (JD2415000 - 29130) [00915];
BD    Cas |since JD2429130 - see Table.
BE    Cas |VB A (B G, 25", 260deg).
BH    Cas |According to [00453] there are no variable stars on the
BH    Cas |place of BH Cas and in its surroundings.
BM    Cas |Min II 8.98. Shape of the light curve varies. P var.
BM    Cas |There is a periodic term in the elements:
BM    Cas |+2.6d*sin(7.11deg*E + 104deg).According to [00939], on the
BM    Cas |light curve cepheid-like variations are observed with
BM    Cas |P = 27d.
BN    Cas |Min II 13.4.
BS    Cas |Min II 12.6.
BU    Cas |D = 0.02P.
BY    Cas |In the region of the cluster NGC 663. P var.
BY    Cas |Max = 2416871.91 + 3.2218d*E (JD2416800 - 24860) [00921];
BY    Cas |Max = 2431929.60 + 3.221297d*E (JD2426900 - 34300);
BY    Cas |Max = 2438399.629 + 3.222588d*E (JD2436200 - 39400);
BY    Cas |since JD2439400 - see Table.
BZ    Cas |Min II 11.5.
CC    Cas |Min II 7.26. The light curve shape var? P var?
CE    CasA|Possible member of the cluster NGC 7790. VB A (B = CEb Cas,
CE    CasA|2.4", 265deg).
CE    CasB|VB B (A = CEa Cas). Possible member of the cluster NGC 7790.
CF    Cas |Possible member of the cluster NGC 7790. [A/H] = 0.1.
CG    Cas |In the region of the cluster NGC 7790.
CH    Cas |[A/H] = -0.5.
CQ    Cas |The slow oscillations are superimposed by more rapid ones
CQ    Cas |with cycles from 110d to 250d.
CR    Cas |Min II 13.3.
CS    Cas |[A/H] = -0.4.
CV    Cas |Epochs given in [00922] are not represented by the elements
CV    Cas |given in the Table. P var?
CW    Cas |Min II 11.47. Shape of the light curve and depths of
CW    Cas |minima vary. P var. Min I = 2435745.6163 + 0.31886497d*E
CW    Cas |(JD2432400 - 41000) [03332]; since JD2441000 - see Table.
CY    Cas |[A/H] = -0.7.
DD    Cas |P var. Max = 2415612.45 + 9.807272d*E (JD2415600 - 18600);
DD    Cas |since JD2418600 - see Table. The star may be a member of a
DD    Cas |binary system with Porb = 8500d +- 1000d.
DF    Cas |In the region of the cluster NGC 1027.
DI    Cas |P var. Max = 2432068 + 371.7d*E (JD2417200 - 32100);
DI    Cas |since JD2432100 - see Table.
DL    Cas |Member of the cluster NGC 129. [A/H] = 0.0.
DN    Cas |Min II 10.13.
DO    Cas |Min II 8.61; dI = 0.08P.
DP    Cas |Min II 13.6.
DZ    Cas |Min II 12.0.
EG    Cas |Min II 13.1.
EK    Cas |Depth of Min II 0.05m.
EM    Cas |P var. Max = 2433132 + 283d*E (JD2427700 - 33150); since
EM    Cas |JD2433150 - see Table. Amplitude strongly varies.
EN    Cas |Min II 12.4. P var.
EP    Cas |Min II 11.4.
EQ    Cas |Min II 12.7. P var. Min I = 2432150.04 + 58.26d*E
EQ    Cas |(JD2432200 - 34060) [03336]; since JD2436100 - see Table.
EY    Cas |Min II 14.5.
GG    Cas |d = 0.013P. Min II 9.99. P var? Min I = 2430188.468 +
GG    Cas |3.758738d*E (JD2424800 - 39500) [00936];
GG    Cas |since JD2439500 - see Table.
GK    Cas |Depth of Min II 0.05m.
GT    Cas |d = 0.02P.
GU    Cas |Min II 11.3. P var. Min I = 2428749.423 + 3.093329d*E
GU    Cas |(JD2417470 - 35480) [00941];
GU    Cas |Min I = 2437367.375 + 3.09325d*E (JD2435480 - 38750) [00001];
GU    Cas |since JD2438750 - see Table.
GZ    Cas |Mean magnitude varies with P = 800d.
GZ    Cas |Max = 2428000 + 800d*E [00911].
HH    Cas |Epoch of Min is given. RV type is possible [00911].
HN    Cas |d = 0.038P.
HS    Cas |VB A (B 12m, 27", 15deg).
HT    Cas |Min hel = 2443727.93722 + 0.073647217d*E;
HT    Cas |D = 0.13P. Depth of eclipses between outbursts is ~2.4 V.
HT    Cas |Small quasi-periodic light oscillations with P = 100s.
HT    Cas |Spectrum description [06163].
HU    Cas |P var. Max = 2417525.075 + 0.41159875d*E (JD2411600 -
HU    Cas |28000); since JD2428000 - see Table.
IL    Cas |Depth of Min II 0.05m.
IR    Cas |Min II 11.5. P var. Min I = 2428750.2914 +
IR    Cas |0.68069178d*E (JD2417500 - 38400) [00098];
IR    Cas |since JD2438400 - see Table.
IS    Cas |Min II 12.2. P var. Min I = 2428776.262 +
IS    Cas |1.8415172d*E (JD2417400 - 29500) [00098];
IS    Cas |since JD2428000 - see Table.
IT    Cas |Min II 11.8; Min II - Min I = 0.553P; DII = 0.042P.
IT    Cas |Apsidal motion is possible.
IV    Cas |Min II 11.3. P var. Min I = 2428991.302 +
IV    Cas |0.9985232d*E (JD2416700 - 29000) [00098];
IV    Cas |Min I = 2431438.648 + 0.9985056d*E (JD2429000 -
IV    Cas |37700) [02263]; since JD2440000 - see Table.
IW    Cas |S4 +/6e.
IX    Cas |P var. Max = 2428749.39 + 9.15035d*E (JD2414700 -
IX    Cas |29500) [00098]; Max = 2428749.90 + 9.1363d*E
IX    Cas |(JD2428700 - 34350) [00944]; Max = 2437195.642 +
IX    Cas |9.14783d*E (JD2434350 - 39100) [05462];
IX    Cas |since JD2442000 - see Table. [A/H] = -0.4.
KL    Cas |Min II 12.3.
KO    Cas |P var. Max = 2425590 + 305.6d*E (JD2416700 - 26000);
KO    Cas |since JD2426000 - see Table.
KR    Cas |Min II 9.9.
LR    Cas |Min II 10.9.
LU    Cas |Min II 14.3?
LW    Cas |In the apex of a small (8") bright cometary nebula in the
LW    Cas |region of IC 1848. Novalike outburst was observed in the
LW    Cas |interval JD2433900 - 34800. Infrared and radioemission.
LX    Cas |In the region of the cluster Collinder 33. Min II 15.3;
LX    Cas |Min II - Min I = 0.47P; dI = 0.10P.
LY    Cas |In the region of the cluster Collinder 33. Min II 15.2.
MM    Cas |d = 0.08P: Min II 12.4.
MN    Cas |Min II 10.57.
MO    Cas |In the nebula NGC 7635. 10.2 - 13.1 I.
MP    Cas |In the nebula NGC 7635. 10.4 - 13.5 I.
MR    Cas |Min II 15.5.
MS    Cas |Min II 13.2.
MT    Cas |d = 0.04P. Min II 14.02.
MU    Cas |Min II 10.8.
MV    Cas |Min II 14.0.
MY    Cas |Min II 15.2. P var. Elements given in the Table are valid
MY    Cas |since JD2438500.
NN    Cas |Min II 14.0.
NT    Cas |Min II 14.4.
NU    Cas |Min II 13.4.
NV    Cas |d = 0.03P.
OP    Cas |P var. Max = 2429109.726 + 5.510019d*E (JD2427950 - 34670)
OP    Cas |[00176]; since JD2437000 - see Table.
OR    Cas |Min II 11.8. P var. Min I = 2429249.424 + 1.2457026d*E
OR    Cas |(JD2413800 - 34800) [00176]; since JD2432000 - see Table.
OX    Cas |In the region of the cluster NGC 381. d = 0.016P. Min II
OX    Cas |10.30; Min II - Min I = 0.512P. Apsidal motion [04524].
PR    Cas |P = 171d?
PV    Cas |Min II 10.36; Min II - Min I = 0.480P.
PV    Cas |Depth of Minima probably varies. P var. Min I =
PV    Cas |2428796.8142 + 1.75047346d*E (JD2415700 - 40000) [05302];
PV    Cas |since JD2440000 - see Table. Apsidal motion [06253]:
PV    Cas |Min II = 2428797.6894 + 1.75047346d*E -
PV    Cas |0.040d*sin(0.0075deg*(E - 3000)).
PX    Cas |Min II 15.0.
PY    Cas |Epoch of Min brighness is given. Similar to RV Tau by
PY    Cas |light curve shape [03348].
PZ    Cas |VB A (B 12.8m, WN 8:, 15", 100deg). OH, H2O emission.
QQ    Cas |Min II 10.8. P var. Min I = 2434330.169 + 2.142030d*E
QQ    Cas |(JD2415700 - 30000) [02530]; since JD2430000 - see Table.
QX    Cas |In the region of the cluster NGC 7790. VB A (B 13.1m, 3").
QX    Cas |Min II 10.50; Min II - Min I = 0.37P; DII = 0.047P;
QX    Cas |dII = 0.018P.
V0336 Cas |Min II 13.6.
V0341 Cas |d = 0.031P.
V0344 Cas |Min II 13.4.
V0345 Cas |Min II 13.6.
V0346 Cas |The coordinates refer to the sp component of a wide pair,
V0346 Cas |whereas the chart [02345] leads to the nf component. It is
V0346 Cas |the sp component that is red and probably var.
V0357 Cas |Min II 13.6.
V0359 Cas |Min II 12.0.
V0360 Cas |Min II 12.3.
V0361 Cas |d = 0.051P.
V0363 Cas |Delta(S) = 1.
V0364 Cas |Min II 11.9.
V0365 Cas |S6/3- .
V0366 Cas |Min II 12.7. P var. Min I = 2435075.461 + 0.7292714d*E
V0366 Cas |(JD2414600 - 35400) [02305]; since JD2434650 - see Table.
V0373 Cas |An unique close binary. Porb = 13.4192d [04627]. Epoch
V0373 Cas |of Min I is given close to the epoch of one of
V0373 Cas |conjunctions. Min II - Min I = 0.58P. Maxima are very
V0373 Cas |sharp. Max - Min II = 0.25P. It is not excluded that the
V0373 Cas |star is an eclipsing one with physical variability of
V0373 Cas |components, but eclipses, if they exist, cause only a very
V0373 Cas |small part of the observed light variations. Range of
V0373 Cas |light variations is given according to [02651]. As a rule
V0373 Cas |the amplitude is close to 0.1m.
V0374 Cas |Min II 12.1.
V0375 Cas |Min II 10.6.
V0377 Cas |VB (A 8.5m; B 9.4m, 2.1", 185deg, 1962).It is not known
V0377 Cas |which component varies. According to [04005] the range
V0377 Cas |of combined brightness variations is 0.26m.
V0377 Cas |According to [07051], const.
V0380 Cas |d = 0.08P.
V0381 Cas |Min II 10.8.
V0388 Cas |Wolf 47 (mu = 0.82", p = 80deg). Faint component of a wide
V0388 Cas |physical pair (p = 294") the bright component of
V0388 Cas |which is the dM2 star Wolf 46 = BD+61deg 195 (9.4).
V0392 Cas |Min II 14.0. P var. Min I = 2429640.390 +
V0392 Cas |4.54094d*E (JD2425300 - 29640); Min I =
V0392 Cas |2429640.390 + 4.54064d*E (JD2429640 - 36900) [04027];
V0392 Cas |since JD2436900 - see Table. Depth of Min var?
V0394 Cas |Min II 15.6.
V0396 Cas |Min II 10.2.
V0399 Cas |Min II 14.1.
V0401 Cas |Min II 15.7.
V0402 Cas |Min II 15.3.
V0406 Cas |Min II 16.8.
V0410 Cas |Bright in 1938 -39. Slow. Not red.
V0423 Cas |Min II 14.3.
V0427 Cas |Min II 13.7.
V0428 Cas |Red.
V0430 Cas |Northern component of a close pair. Red.
V0434 Cas |Red.
V0441 Cas |P = 351.2d?
V0442 Cas |d = 0.025P. P var? Since 1972 P = 3.592120d.
V0444 Cas |Min II 16.0. P var. Min I = 2438651.314 + 2.224808d*E
V0444 Cas |(JD2432850 - 37300); since JD2437300 - see Table. Period
V0444 Cas |variation may be cyclic. Mean elements:
V0444 Cas |Min I = 2443194.258 + 2.224773d*E.
V0445 Cas |Min II 11.08.
V0448 Cas |Min II 15.0.
V0450 Cas |VB A (B 17.5m:, 3.4", 188deg). Range
V0450 Cas |of combined light variations is given.
V0459 Cas |Min II 11.6.
V0466 Cas |In the region of the cluster NGC 457.
V0480 Cas |Min II 14.7.
V0482 Cas |VB A (B 10.0m, F 4 V, 6", 195deg; optical). P = 0.28292d?
V0497 Cas |In the region of the cluster IC 1848.
V0498 Cas |In the region of the cluster IC 1848.
V0499 Cas |In the region of the cluster IC 1848.
V0509 Cas |Pulsation of photosphere with P = 3 years.
V0509 Cas |Tenuous shell ejected in 1975 is now falling back to
V0509 Cas |the star.
V0518 Cas |In the region of the cluster Stock 2. Star N136 (Stock 208).
V0520 Cas |Min II 13.1. P var. Min I = 2439069.559 + 0.489832d*E
V0520 Cas |(JD2438580 - 40850); since JD2441150 - see Table.
V0521 Cas |Member of the cluster NGC 7789.
V0523 Cas |Min II 11.34. P var. Min I = 2432054.555 +
V0523 Cas |0.2336882d*E (JD2428545 - 33570) [07008];
V0523 Cas |Min I = 2439029.461 + 0.23368912d*E (JD2439000 - 41300)
V0523 Cas |[07387]; since JD2440480 - see Table.
V0524 Cas |OH, H2O emission. P = 163d?, 191d? 259d?, 620d?
V0526 Cas |Two oscillations are superimposed: P1 = 0.0526d (A1 =
V0526 Cas |0.0036m), P2 = 0.0396d (A2 = 0.0056m); P2/P1 = 0.753.
V0527 Cas |Min II 13.5; Min II - Min I = 0.52P.
V0532 Cas |In the region of the cluster NGC 7789.
V0533 Cas |In the region of the cluster NGC 7789.
V0536 Cas |P var. Max = 2438700.262 + 0.395674d*E
V0536 Cas |(JD2438580 - 39150); Max = 2441186.333 +
V0536 Cas |0.395683D*E (JD2440070 - 41250);
V0536 Cas |since JD2441500 - see Table.
V0540 Cas |Epoch of Max (U) is given.
V0541 Cas |Min II 11.0.
V0542 Cas |In the region of the cluster NGC 7789.
V0544 Cas |Elements given in the Table are valid since JD2428000.
V0546 Cas |In the region of the cluster NGC 103. Min II 14.8.
V0547 Cas |VB A (B 12.4m, M4.5, 2.8", 93deg). Astrometric binary
V0547 Cas |(A = 0.12", P = 15.9a); mu = 1.75", P = 98deg.
V0547 Cas |Variation of combined light is given.
V0551 Cas |P = 45.5d?/57d?/67.5d?.
V0554 Cas |P >= 3500d? D = 400d?
V0559 Cas |VB A (B 7.7m, 0.25", 34deg, 1976). Min II 7.21.
V0566 Cas |VB A (B 8.3m, 1.4", 194deg, 1965).
V0569 Cas |10.0 - 14.7 I.
V0589 Cas |In the cluster NGC 663.
V0592 Cas |White dwarf. Rapid non-periodic fluctuations of brightness
V0592 Cas |on a time scale of several minutes.
V0598 Cas |VB A (B 12m, 19", 0deg). P = 2.825d? [02560].
V0615 Cas |Variable radio source on 10.5 GHz; gamma - and X-ray
V0615 Cas |source?
V0627 Cas |H2O emission.
V0635 Cas |4U 0115 + 634. SB (P = 24.3162d).
V0635 Cas |Pulsar period P = 3.6136s.
V0638 Cas |Epoch of Min is given.
V0742 Cas |SB, Porb = 55.9212d.
V0745 Cas |Component B of the double system observed brighter than in the
V0745 Cas |Hipparcos Input Catalogue.
V0746 Cas |SB, Porb = 27.8d.
V0747 Cas |VB. The variability may be due to the fainter component.
alf   Cas |VB A (B 14.5m, 17.6", 272deg; C 13.5m, 38", 105deg;
alf   Cas |D 8.5m, 64.4", 280deg.)
bet   Cas |VB A (B 13.7m, 31.3", 243deg); SB (P = 27d).
bet   Cas |[Fe/H] = 0.64.
gam   Cas |VB A (B 11.0m, 2.2", 248deg; C 13.0m, 52.2", 348deg).
gam   Cas |In HII region S 185. X-ray source MX 0053 + 60.
gam   Cas |v sin i = 310 km/s.
del   Cas |VB A (B 11.5m, 31.7", 66deg). Min II 2.75. Min II - Min I =
del   Cas |361d. The elements given in the Table are still not
del   Cas |confirmed by anyone.
iot   Cas |VB A (B 6.89m, 2.3", 239deg; C 8.40m, 7.2", 114deg).
iot   Cas |Astrometric binary (a = 0.113", P = 52.4a). Max (V) - Max
iot   Cas |(lambda 1550) = 0.4P; A (lambda 1550) = 0.40m. The range
iot   Cas |of total brightness variation of components A and
iot   Cas |B is given.
kap   Cas |P = 0.09028d, P(Vr) = 0.14035d [02588]; P = 7d [08876].
omi   Cas |VB A (B 11.7m, 33.6", 303deg). SB1 (P = 1033d);
omi   Cas |V sin I = 220 km/s.
pi    Cas |SB, Porb = 1.9642d.
rho   Cas |Usually varies within the limits 4.4m - 5.2m V.
rho   Cas |In November 1945 the peculiar decrease of brightness began
rho   Cas |lasting for 165d and in September 1946 the star reached
rho   Cas |the middle of the deepest minimum (JD2432070) lasting for
rho   Cas |320d. Then the brightness began to increase symmetrically
rho   Cas |and by July 1947 the star attained its normal brightness
rho   Cas |[00957]. Photographic magnitudes varied in the limits
rho   Cas |5.4m - 8.3m. Spectrum description [08878].
B     Cas |Tycho Brahe's supernova. Stellar object is not identified
B     Cas |optically up to now.
R     Cen |VB A (B 12m, 28", 218deg). Epoch
R     Cen |of Min I is given. Min I 0.00P, Max I 0.23P, Min II
R     Cen |0.47P, Max II 0.64P. <Max I> 5.8, <Max II> 6.0,
R     Cen |<Min I> 11.1, <Min II> 8.3. P var. P = 561.3d
R     Cen |before 1918; since 1918 - see Table. H2O maser.
V     Cen |In the field of the open cluster NGC 5662.
Z     Cen |SN 1895 (NGC 5253).
RR    Cen |Min II 7.63. dII = 0.08P. P var. Min I = 2424231.0910 +
RR    Cen |0.60568807d*E + 2.31d*10**(-10)*E**2 (JD2414170 -
RR    Cen |33470) [00006]. Current elements - see Table.
RS    Cen |A 1118-61?
RT    Cen |P var.
RZ    Cen |Min II 9.4.
SS    Cen |Min II 9.5.
ST    Cen |Min II 11.30, DII = 0.22P. Max II (before
ST    Cen |Min I) 10.65.
SU    Cen |Min II 9.2.
SV    Cen |Min II 9.45. Delta(m) var. P var. Min = 2433053.358 +
SV    Cen |1.6594795d*E - 7.61d*10**(-8)*E**2 (JD2412608 - 42097).
SV    Cen |Cyclic (32a - 33.6a) period variations were noted in
SV    Cen |[00009,05212]. Since 1978 - see Table. P Cyg profiles in
SV    Cen |the spectrum.
SX    Cen |For mean light Max = 2426835 + 615d*E.
SY    Cen |d = 0.05P.
SZ    Cen |VB. Min II 8.7.
TX    Cen |VB? B - V: +1.39, +2.11.
TZ    Cen |The co-ordinates in the Table are based on [00015].
TZ    Cen |According to [00016], no star brighter than 14m was found
TZ    Cen |in this position. The co-ordinates in [00015] may be in
TZ    Cen |error.
UW    Cen |IR excess.In Max varies semiregularly, P ~42d [08832].
UZ    Cen |VB A (B 13.8m, 4", 191deg). Max II = 2440746.2 +
UZ    Cen |2.35529d*E.
VW    Cen |VB A (B ~15m?, ~8", ~180deg). B - V: +1.01, +1.71.
VW    Cen |[A/H] = 0.3.
VZ    Cen |Min II 8.4.
WX    Cen |<B - V> ~ +0.45, <U - B> ~ -0.72.
WX    Cen |Proposed as an optical counterpart of the transient X-ray
WX    Cen |source Cen X-2 [05314], though no optical bursts were
WX    Cen |observed.
WZ    Cen |Min II 14.2.
ZZ    Cen |VB C (A 9.4m, B9; B 10.8m, 8", 314deg; C = ZZ Cen,
ZZ    Cen |9", 259deg; D = AA Cen, 9", 110deg).
AA    Cen |VB D (see ZZ Cen).
AB    Cen |d = 0.05P.
AP    Cen |Epoch of Min is given.
AS    Cen |Min II 13.2.
AV    Cen |Min II 14.1.
AZ    Cen |The shape of the light curve varies.
BD    Cen |Min II 10.7.
BF    Cen |In the field of the open cluster NGC 3766. Min II 8.8.
BG    Cen |Min II 12.3.
BH    Cen |In the open cluster IC 2994. Min II 8.8.
BI    Cen |Delta(S) = 2.
BK    Cen |P2 = 2.236d, A1 = 0.54m, A2 = 0.22m [08835].
BV    Cen |The mean cycle between outbursts <= 149.4d [07301]. The
BV    Cen |tabulated elements correspond to Max of the eclipsing
BV    Cen |light curve, phi (Min) = 0.25P. The range of the eclipsing
BV    Cen |variability is 12.8 - 13.3.
CN    Cen |Min II 13.3.
DI    Cen |Min II 12.3, Min II - Min I = 0.494P, DII = 0.08P:.
DT    Cen |Red.
DX    Cen |The P star in a pair.
DY    Cen |All spectral lines are very weak. No IR excess. The
DY    Cen |photometric behaviour outside major Min is described in
DY    Cen |[08836].
EP    Cen |Min II 11.5.
EU    Cen |The P star in a pair.
GI    Cen |In the field of the globular cluster NGC 5286.
GM    Cen |The chart in [06286] is wrong.
IQ    Cen |d = 0.04P.
IW    Cen |Min II 12.1.
IX    Cen |In the field of the open cluster NGC 3706.
IY    Cen |In the field of the open cluster IC 2944.
IZ    Cen |<B - V> = 1.7.
KK    Cen |B - V: +1.08, +1.62.
KM    Cen |Min II 13.3.
KN    Cen |B - V: +1.36, +1.75. [A/H] = 0.2.
KQ    Cen |Alternating periods 136d, 159d.
KT    Cen |B - V: +0.46. Min II 12.72. Min II - Min I = 0.392P
KT    Cen |(JD2441686 - 721); apsidal motion is observed [08094].
KY    Cen |Min II 13.3.
KZ    Cen |B - V: +0.30, +0.72.
LL    Cen |Min II 13.1.
LR    Cen |Min II 12.30.
LT    Cen |Min II 9.6.
LU    Cen |The period may be twice longer.
LV    Cen |B - V: +1.3, +1.7.
LW    Cen |Min II 9.6. In the field of the open cluster IC 2944.
LX    Cen |Min II 13.55.
LZ    Cen |Min II 8.50.
MM    Cen |Min II 12.7.
MN    Cen |Min II 8.7. VB A (B 10.9m, 7", 147deg).
MP    Cen |Min II 10.0.
MQ    Cen |Min II 10.1.
MR    Cen |Min II 10.5.
MV    Cen |Min II 14.6.
MY    Cen |B - V: +1.58, +1.94.
NO    Cen |Min II 14.2.
NP    Cen |Min II 10.2.
NY    Cen |Min II 11.9.
OO    Cen |<B - V> = 1.84.
OP    Cen |Min II 13.8.
OU    Cen |Min II 10.9.
OV    Cen |Min II 11.0.
OX    Cen |Min II 14.3.
QS    Cen |d = 0.03P.
QT    Cen |Min II 13.4.
QY    Cen |<B - V> = 2.16.
QZ    Cen |P var? The shape of the light curve varies?
V0339 Cen |VB A (B ~13m, SP). B - V: +1.08, +1.47.
V0343 Cen |Min II 13.5.
V0344 Cen |Min II 12.3.
V0346 Cen |In the field of the open cluster Stock 14. Min II 8.8.
V0346 Cen |Min II = 2421966.835 + 6.32189d*E.
V0348 Cen |d = 0.010P.
V0349 Cen |Min II 14.5.
V0350 Cen |Min II 10.3. Min II = 2430870.192 + 3.216906d*E.
V0351 Cen |Epoch of Min is given.
V0356 Cen |Min II 15.0.
V0358 Cen |Epoch of Min is given.
V0365 Cen |d = 0.040P.
V0373 Cen |VB A (B ~4" np).
V0377 Cen |d = 0.003P.
V0379 Cen |Min II 8.9.
V0380 Cen |Min II 10.0.
V0383 Cen |Min II 13.6:, Min II - Min I = 0.609P.
V0384 Cen |Min II 12.2. DII = 0.062P. Min II - Min I = 0.667P.
V0385 Cen |Min II 13.0.
V0388 Cen |Min II 15.7.
V0399 Cen |d = 0.020P. Min II 13.1.
V0405 Cen |P var, 30d - 40d.
V0412 Cen |VB A (B 59", 266deg).
V0419 Cen |P var. Max = 2428099.25 + 5.50713d*E (JD2428099 - 33573);
V0419 Cen |since JD2434900 - see Table.
V0420 Cen |B - V: +0.45, +0.97. P var. Nonlinear term:
V0420 Cen |-0.000090d*E**2.
V0427 Cen |Epoch of Min is given.
V0436 Cen |SB (P = 0.0669d). Photometric P during supermaxima
V0436 Cen |0.06383d [08838]. Rapid oscillations in supermaxima
V0436 Cen |Delta(m) ~0.002m, P ~19.6s [08049].
V0440 Cen |d = 0.033P. Min II is possible.
V0443 Cen |d = 0.025P.
V0491 Cen |Very flat minima; close companion?
V0495 Cen |d = 0.042P. Min II 10.6. Min II - Min I = 0.520P.
V0496 Cen |Possible member of the open cluster NGC 4755.
V0496 Cen |B - V: +1.02, +1.33.
V0498 Cen |P may be twice shorter.
V0499 Cen |(k - b)2 = 0.23.
V0504 Cen |Semiregular  variations (P1 ~130d, P2 ~411d)
V0504 Cen |are also observed [08836].
V0506 Cen |The chart in [06286] is wrong.
V0508 Cen |Min II 13.2.
V0526 Cen |Delta(m) var. P var. Max = 2425707.540 + 0.56153d*E
V0526 Cen |(1929 - 1930); during 1931 - 1940 - see Table.
V0527 Cen |The chart in [06286] is wrong.
V0532 Cen |Star 1 [09078]. X-ray source 3A 1431-409.
V0544 Cen |2AS E 1440-39? [05962]. The chart in [06286] is wrong.
V0545 Cen |Magnitude in Max var (12.6 - 14.5), P = 1800d?
V0553 Cen |[Fe/H] = -0.1; [C/Fe] = +0.8.
V0565 Cen |Min II 13.9. Type RR is not excluded (P = 0.238072d).
V0574 Cen |sp star of a pair.
V0577 Cen |According to improved coordinates, the star is actually in
V0577 Cen |Hydra.
V0585 Cen |Min II 13.0.
V0592 Cen |Mean brightness var.
V0593 Cen |Possible member of the open cluster Stock 16. Min II 11.2.
V0594 Cen |V133 (omega Cen); non-member of the cluster. Min II 14.4.
V0606 Cen |Min II 9.8.
V0607 Cen |Min II 14.1.
V0608 Cen |Min II 13.1.
V0609 Cen |Min II 13.6.
V0615 Cen |Min II 14.0.
V0617 Cen |Min II 13.8:.
V0619 Cen |In the field of the open cluster NGC 5316.
V0621 Cen |d = 0.05P.
V0624 Cen |Min II 14.9.
V0625 Cen |Min II 15.0.
V0627 Cen |d = 0.02P.
V0628 Cen |Min II 13.2.
V0630 Cen |Min II 14.2. d = 0.06P.
V0635 Cen |Min II 13.9.
V0636 Cen |Min II 8.8.
V0644 Cen |During the faint phase in 1951 the shell spectrum was
V0644 Cen |observed [02128]. Type E with a very long period is
V0644 Cen |possible [06763].
V0645 Cen |Proxima Cen = alpha Cen C. mu = 3.809", P = 281.7deg.
V0645 Cen |Soft X-ray source.
V0646 Cen |d = 0.022P. Min II 9.1.
V0662 Cen |P ~2.48d or 2.95d.
V0672 Cen |Min II 11.4 - 11.6 (var).
V0673 Cen |Depth of Min II 0.05m.
V0674 Cen |Blazhko effect: Pi = 29.5d. 0.15P <= M - m <= 0.23P.
V0676 Cen |Min II 12.5.
V0677 Cen |Min II 11.6.
V0678 Cen |Min II 10.6.
V0679 Cen |9.8"p, 1.1"n from CPD -62deg 2167.
V0679 Cen |The star is at the edge of a dark cloud in a bright nebula,
V0679 Cen |a part of IC 2944, in the field of a very poor open
V0679 Cen |cluster. Since 1950 till 1954 faded by 2.5m. Rather red.
V0679 Cen |"Screening" by the edge of a dark nebula?
V0682 Cen |IR excess.
V0684 Cen |Depth of Min II 0.05m.
V0685 Cen |Min II 9.5.
V0686 Cen |RV type is not excluded.
V0687 Cen |Min II 14.1. DII = 0.12P. Min II - Min I = 0.580P.
V0688 Cen |Min II 12.7.
V0689 Cen |Min II 12.1.
V0690 Cen |Depth of Min II 0.03m.
V0692 Cen |Min II 11.6. Min II - Min I = 0.481P.
V0701 Cen |VB? d = 0.026P. Min II 9.1.
V0704 Cen |IR excess.
V0716 Cen |Min II 6.21.
V0742 Cen |Min II 10.1.
V0743 Cen |(k - b)2 = 0.20. Elements almost as well satisfactory:
V0743 Cen |Max = 2439243.6465 + 0.10222560d*E.
V0745 Cen |Min II 9.6.
V0746 Cen |= V467 Cen. Marked as V467 Cen in the chart.
V0747 Cen |Min II 10.05.
V0748 Cen |B - V: +0.31, +1.21; U - B: -0.66, -0.21. d = 0.106P.
V0748 Cen |Narrow Halpha emission. Outside eclipses shows variations
V0748 Cen |by 0.05m - 0.1m during several days or several weeks
V0748 Cen |(probably irregularly) [06968].
V0752 Cen |Min II 9.61. dI = dII = 0.047P.
V0753 Cen |(k - b)2 = 0.20. In the field of the open cluster NGC 3960;
V0753 Cen |probably non-member. Type DSCT is possible.
V0754 Cen |Slight Min II.
V0755 Cen |In the Coalsack.
V0756 Cen |In the Coalsack. High excitation lines (OVII, OVIII, CV)
V0756 Cen |are present in the spectrum. WR type is possible [07372].
V0757 Cen |Min II 8.6.
V0758 Cen |d = 0.07P. Min II 9.15.
V0759 Cen |Min II 7.56.
V0761 Cen |IR excess.
V0763 Cen |VB A (B 13m, 7", 163deg).
V0766 Cen |VB A (B 10.01m, B0Ibp, 9", 318deg). IR excess.
V0767 Cen |VB A (B 11.52m, 21", 350deg).
V0768 Cen |Possible P: 60d - 80d.
V0770 Cen |According to [07570], const?
V0772 Cen |In the region of the open cluster IC 2944.
V0775 Cen |EB type is possible. Deep Min II.
V0777 Cen |Deep Min II.
V0779 Cen |Cen X-3 (3U 1118-60). <B - V>: +1.04; <U - B>:  -0.08.
V0779 Cen |Min II 13.39. Porb var. The shape of the light curve
V0779 Cen |varies. Epoch of Min I is given. Epochs of Min II coincide
V0779 Cen |with the moments of X-ray eclipses. X-ray pulses are
V0779 Cen |observed with Ppuls = 4.834477s (epoch JD2442785.3);
V0779 Cen |Ppuls decreases [07612]. No rapid optical oscillations
V0779 Cen |were found.
V0783 Cen |B - V: +0.35.
V0784 Cen |Very red.
V0788 Cen |Min II 5.90.
V0790 Cen |VB B (A 4.52m; 60", 343deg).
V0791 Cen |In the region of globular cluster omega Cen (NGC 5139).
V0791 Cen |Cluster non-member.
V0795 Cen |VB A (B 12.29m, 33.9", 170deg; C 12.79m, 36", 220deg).
V0801 Cen |4U 1145 - 61 = 2S 1145 - 619. Primary component has a low
V0801 Cen |density envelope expanding with the velocity of 1800 km/s.
V0801 Cen |V sin i = 290 km/s. X-ray pulsar (P = 291.8s
V0801 Cen |[08883]). Max (X) = 2442519.5 + 187.5d*E [08881].
V0803 Cen |Extremely hot hydrogen-deficient helium star.
V0807 Cen |VB (9.9m, 10.1m, 0.4", 258deg, 1931).
V0807 Cen |It is not known which of the components varies.
V0810 Cen |Member of the cluster Stock 14.
V0813 Cen |In the region of globular cluster omega Cen (NGC 5139).
V0813 Cen |V65 (NGC 5139).
V0814 Cen |In the region of globular cluster omega Cen (NGC 5139).
V0814 Cen |V78 (NGC 5139). Min II 14.165:. Primary
V0814 Cen |component is probably intrinsically variable [08884].
V0816 Cen |Primary oscillation is superimposed by the oscillations
V0816 Cen |with freguencies: F2 = 4.9229, F3 = 4.7343, F4 = 4.9317
V0816 Cen |[02591].
V0820 Cen |[Fe/H] = -2.5; Vr = +260 km/s.
V0822 Cen |Cen X-4.
V0825 Cen |In the region of globular cluster omega Cen (NGC 5139).
V0825 Cen |Cluster non-member. V2 (NGC 5139).
V0826 Cen |In the region of globular cluster omega Cen (NGC 5139).
V0826 Cen |Cluster non-member. V129 (NGC 5139).
V0902 Cen |VB, rho = 12". Variability may be spurious.
V0915 Cen |The variability type is not quite consistent with the spectral
V0915 Cen |type (B9II/III).
V0921 Cen |High proper motion (LTT 4397) not confirmed by HIPPARCOS data.
V0933 Cen |HIPPARCOS data contradict the luminosity class V.
V1015 Cen |Variability type and luminosity class (III) do not agree.
V1045 Cen |Background field star.
bet   Cen |VB A (B 4.1m, 1.3", 251deg, 1960). SB1 (P = 352d
bet   Cen |[08887]. Multiperiodicity; sometimes brightness is constant
bet   Cen |[08215]. Soft X-ray source.
del   Cen |VB A (B 4.8m, 68.6", 325deg; C 6.5m, 16.6", 227deg).
eps   Cen |VB A (B 13.0m, 36.0", 158deg). There is a secondary light
eps   Cen |oscillation with the amplitude of 0.0034m and elements:
eps   Cen |Max = 2441041.058 + 0.17696d*E.
eta   Cen |VB A (B 13.5m, 5.6", 270deg, 1897); SB?
mu    Cen |VB A (B 13.63m, 48", 128deg).
omi 1 Cen |VB A (B 11.4m, 13.5", 125deg).
T     Cep |P var. Max = 2414252 + 386.05d*E (JD2406900 - 20490);
T     Cep |Max = 2431086 + 394.93d*E (JD2420490 - 32900);
T     Cep |Max = 2440262 + 379.22d*E (JD2432900 - 42200); since
T     Cep |JD2442200 Max = 2444171 + 392.7d*E. Mean value of the
T     Cep |period is given in the Table. SiO maser.
U     Cep |VB A (B 11.83m, 13.9", 62deg; C 12.3m, 23.0", 318deg).
U     Cep |0.010P <= d <= 0.040P. Min II 6.93. P var. Min I =
U     Cep |2407890.3346 + 2.4928551d*E + 5.15d*10**(-9)*E**2
U     Cep |(JD2388855 - 2440790) [06468]; analysis of period
U     Cep |variations in this interval see also in [07395];
U     Cep |Min I = 2441395.3604 + 2.4931048d*E (JD2440790 - 41600);
U     Cep |Min I = 2441679.5716 + 2.4930432d*E (JD2441600 - 950);
U     Cep |Min I = 2443753.7982 + 2.4930679d*E (JD2442100 - 43800);
U     Cep |since JD2444000 - see Table. Shape of the light curve
U     Cep |and depth of minima vary. Brightness of the secondary (G8)
U     Cep |varies sporadically. Subgiant brightening accompanies
U     Cep |eruptive mass transfer. The gaseous stream moving to the
U     Cep |primary (B7) component forms around it gaseous ring or
U     Cep |disc [08889].
W     Cep |Slow oscillations with Pi ~2000d are superimposed by
W     Cep |oscillations with P ~350d.
X     Cep |OH emission?
RS    Cep |d = 0.039P. P var. Min = 2417140.469 + 12.419925d*E
RS    Cep |(JD2410000 - 31000) [02431]; since JD2431000 - see Table.
RZ    Cep |P var. Max = 2411640.654 + 0.308697d*E
RZ    Cep |(JD2411640 - 15000); Max = 2417144.620 + 0.3086203d*E
RZ    Cep |(JD2415600 - 20200); Max = 2421175.611 +
RZ    Cep |0.3086699d*E (JD2421175 - 23000); Max =
RZ    Cep |2423768.475 + 0.3086918d*E (JD2423000 - 31700);
RZ    Cep |Max = 2433768.493 + 0.3086383d*E (JD2433700 -
RZ    Cep |38300) [08890]; Max = 2438207.938 + 0.308645d*E
RZ    Cep |(JD2438200 - 39040) [03879]; Max = 2440834.579 +
RZ    Cep |0.3086735d*E (JD2440800 - 42640) [08890];
RZ    Cep |since JD2442640 - see Table. Shape of the light curve and
RZ    Cep |the amplitude A vary with the Blazhko effect period
RZ    Cep |Pb = 96.8*P0 = 29.88d; Min A = 2441464.147 + 29.88d*N
RZ    Cep |[08891]. Long period variation of P0 with a period ~50
RZ    Cep |years is possible. Delta(S) = 6.
SS    Cep |Mean brightness varies with cycles from some hundreds to
SS    Cep |thousands days.
SU    Cep |Min II 10.6.
SV    Cep |IR excess.
SX    Cep |In the region of the nebula NGC 7023.
SY    Cep |Min II 12.70. P var?
SZ    Cep |VB A (B 12.3m, 24.9", 263deg). S4/6e.
TT    Cep |VB A (B 17.0m, 8", 160deg).
TY    Cep |Epoch of Min I is given.
UZ    Cep |P var. Max = 2440969 + 297.68d*E (JD2414000 - 42000);
UZ    Cep |since JD2440000 - see Table.
VV    Cep |VB (0.05", 174deg, 1950)? 0.066P <= D <= 0.091P;
VV    Cep |0.040P <= d <= 0.077P. Depth of eclipses: 2.30m (lambda
VV    Cep |3500 A), 1.9m (U), 0.4m (B). M-component is of SRC type:
VV    Cep |Max = 2443045 + 118.37d*E [08698,08894]; A(V) <= 0.33m.
VV    Cep |Light oscillations are also noted with P ~58d [08895],
VV    Cep |25d and 150d [08896]. B-component may be also an intrinsic
VV    Cep |variable [02416]. Gaseous streams. Strong variable magnetic
VV    Cep |field.
VW    Cep |VB A (B 10.3m, a = 0.51", P = 30.45a [08897]); mu alpha =
VW    Cep |+0.0899s, mu delta = +0.560". Min II 7.56.
VW    Cep |Shape of the light curve and depths of Min I and Min II
VW    Cep |vary. P var. Min I = 2433483.4257 + 0.27831758d*E +
VW    Cep |0.050d*cos(0.004813deg*(E - 4700)) (JD2424763 - 41200)
VW    Cep |[06483]; since JD2441000 - see Table. Period
VW    Cep |change study see also in [08899]. X-ray source.
VZ    Cep |Min II 9.93.
WX    Cep |Min II 9.14; dI = 0.01P, dII = 0.00P.
WY    Cep |Min II 11.5. P var [02545].
WZ    Cep |Min II 11.9.
XX    Cep |Min II 9.26. P var. Min I = 2425096.449 + 2.337340d*E
XX    Cep |(JD2414930 - 30000); Min I = 2441539.4917 + 2.3373059d*E
XX    Cep |(JD2430000 - 42300) [08902]. Since JD2441500 - see Table.
XY    Cep |Min II 10.10. P var?
XZ    Cep |Min II 8.43.
ZZ    Cep |VB A (B 10.2m, A2 P, 3.6", 202deg; C 10.87m, A5V,
ZZ    Cep |20.6", 219deg). Min II 8.74.
AH    Cep |Min II 7.03. Depth of minima varies. P var.
AH    Cep |Min I = 2434989.3702 + 1.7747274d*E (JD2415500 - 35000)
AH    Cep |[03604]; since  JD2434900 - see Table: +3.12d*10**(-9)*E**2.
AI    Cep |Min II 9.48.
AN    Cep |Since JD2425200 primary and secondary maxima and minima
AN    Cep |appeared, and mean cycle became 254d.
AV    Cep |d <= 0.04P.
BB    Cep |d = 0.050P.
BE    Cep |Min II 13.0.
BF    Cep |P var. Max = 2437236 + 426.11d*E (JD2423600 - 37300);
BF    Cep |Max = 2441665 + 442.3d*E (JD2437300 - 42500); since
BF    Cep |JD2442500 - see Table.
BH    Cep |Sometimes strong Algol-like light weakenings are observed.
BO    Cep |Sometimes strong Algol-like light weakenings are observed.
CO    Cep |Min II 12.6; Min II - Min I = 0.552P; DII = 0.080P.
CP    Cep |P var?
CQ    Cep |Shape of the light curve and depth of minima vary.
CQ    Cep |According to [07401] on 1969 March 28/29 on the phase
CQ    Cep |0.56P a light decrease by 0.1m was observed and then a
CQ    Cep |rapid flare by 0.35m U, 0.13m B, 0.14m V. P var. Nonlinear
CQ    Cep |term: -10**(-9)*E**2.
CR    Cep |P var. Max = 2436846.94 + 6.23318d*E (JD2415000 - 30000)
CR    Cep |[03157]; since JD2430000 - see Table.
CV    Cep |S7/1.5. Mean brightness varies with a cycle ~2000d [00159].
CW    Cep |VB A (B 12.29m, 20", 310deg). Min II 8.01;
CW    Cep |Min II -  Min I = 0.478P (1972 yr). There is a sinusoidal
CW    Cep |term in the elements: +0.0250d*sin(0.0626deg*E - 28.3deg).
CW    Cep |Apsidal motion with P = 43a.
CX    Cep |Min II 12.16.
CY    Cep |Min II 16.5.
DD    Cep |P var. Max = 2427960 + 167.6d*E (JD2427900 - 30000);
DD    Cep |Max = 2429968 + 173.0d*E (JD2429900 - 33600);
DD    Cep |since JD2433600 - see Table.
DH    Cep |In the region of the cluster NGC 7380. Apsidal motion with
DH    Cep |P = 2.6a [00165].
DK    Cep |Min II 12.4.
DL    Cep |Min II 12.7.
DO    Cep |VB B (A 9.87m, M4V; a = 2,4", P = 44.78a, e = 0.408);
DO    Cep |mu = 0.852", P = 242.6deg.
DP    Cep |Min II 14.4.
DQ    Cep |Multiperiodicity: P0 = 0.12420d: [08137], P1 = 0.061177d
DQ    Cep |[08914].
DX    Cep |P var. Max = 2430603.712 + 0.5260395d*E (JD2415700 - 31000)
DX    Cep |[00001]; since JD2431000 - see Table. Delta(S) = 7.
DY    Cep |Min II 11.8.
EE    Cep |A var?
EF    Cep |Min II 12.6. P var?
EG    Cep |Min II 9.61. P var. Min I = 2439774.3322 + 0.54462091d*E
EG    Cep |(JD2415200 - 41000) [00001]; since JD2441000 - see Table.
EH    Cep |In the dark cloud near the diffuse nebula and the cluster
EH    Cep |NGC 7023.
EI    Cep |Min II 7.98.
EK    Cep |Min II 8.06; Min II - Min I = 0.545P (1965). Min II =
EK    Cep |2439022.8484 + 4.427797d*E [08160].
EK    Cep |Apsidal motion (P = 4700a  +- 600a) [08923].
EL    Cep |P var.
EM    Cep |In the region of the cluster NGC 7160. VB A (a 12.8m,
EM    Cep |19.8", 281deg; B 7.9m, 62.5", 146deg). Min II 7.16.
EM    Cep |Shape of the light curve and depth of minima vary.
EO    Cep |Min II 12.3.
EP    Cep |In the cluster NGC 188. Min II 17.0.
EQ    Cep |In the cluster NGC 188. Min II 16.7.
ER    Cep |In the cluster NGC 188. Min II 16.27.
ES    Cep |In the cluster NGC 188. Min II 15.8.
ES    Cep |P var. Min I = 2439082.238 + 0.34468d*E (JD2438480 - 39090);
ES    Cep |Min I = 2439236.501 + 0.34264d*E (JD2439090 - 39280);
ES    Cep |Min I = 2439594.548 + 0.34250d*E (JD2439400 - 39600);
ES    Cep |since JD2439600 - see Table. A var.
EX    Cep |Min II 11.6.
EY    Cep |Min II 10.4.
EZ    Cep |P var. Max = 2416803.627 + 0.378990d*E (JD2415400 - 20000)
EZ    Cep |[00001]; since JD2420000 - see Table.
FH    Cep |Min II 12.1.
FL    Cep |d = 0.02P.
FS    Cep |Min II 12.0.
FT    Cep |VB A (B 18.3m, 5", 27deg). In the region of the diffuse
FT    Cep |nebula and the cluster NGC 7023.
FU    Cep |In the region of the diffuse nebula and the cluster
FU    Cep |NGC 7023.
FV    Cep |In the region of the diffuse nebula and the cluster
FV    Cep |NGC 7023. P = 0.4628d.
FW    Cep |In the region of the diffuse nebula and the cluster
FW    Cep |NGC 7023.
GI    Cep |Min II 11.9.
GK    Cep |Min II 7.35; dI = dII = 0.03P; Min II - Min I = 0.502P.
GK    Cep |P var. Min I = 2425189.526 + 0.9361614d*E
GK    Cep |(JD2415000 - 27500); Min I = 2438694.7070 + 0.9361714d*E
GK    Cep |(JD2427500 - 38200) [00001]; since JD2438200 - see Table.
GL    Cep |In the region of the diffuse nebula IC 1396 and the
GL    Cep |cluster Tr 37.
GM    Cep |In the region of the diffuse nebula IC 1396 and the
GM    Cep |cluster Tr 37.
GP    Cep |In the region of the HII zone S 132. Quadruple system,
GP    Cep |consisting of a WN6 + O8-B0III: eclipsing pair
GP    Cep |(P = 6.6883d) physically associated with an O + O pair
GP    Cep |(P = 3.4698d); the latter pair may be also an eclipsing
GP    Cep |or ellipsoidal variable [08931].
GS    Cep |Min II 10.6.
GT    Cep |Min II 8.6.
GW    Cep |Min II 12.00.
HK    Cep |Min II 14.4.
HZ    Cep |In the region of the diffuse nebula and the cluster
HZ    Cep |NGC 7023.
IL    Cep |VB A (B 11.91m, 7", 326deg); P = 2.802d?
IM    Cep |Min II 13.6.
IO    Cep |Min II 11.7.
IP    Cep |Min II 12.1.
IR    Cep |VB (Delta(m) ~0.0m, 0.0" -0.2"). P var.
IR    Cep |Max = 2431060.878 + 2.114016d*E (JD2428335 - 31060) [00001];
IR    Cep |since JD2440900 - see Table.
IV    Cep |VB B (A 16m; B 2.1", 191deg).
IW    Cep |Min II 13.7; Min II - Min I = 0.52P.
IX    Cep |d = 0.03P. Min II 17.0.
KL    Cep |d = 0.019P.
KP    Cep |Depth of Min II 0.03m.
KV    Cep |Min II 14.3.
KY    Cep |Flare with 65 sec duration. There is a blue object on the
KY    Cep |place of the flare [00001].
KZ    Cep |VB (8.6m, 8.6m; 1.9", 348deg). Depths of spectral lines
KZ    Cep |vary: P = 0.212938d [06488].
LL    Cep |Min II 14.0.
LM    Cep |Min II 12.8.
LP    Cep |Min II 13.8; Min II - Min I = 0.55P.
LQ    Cep |Eastern component of a double star.
LU    Cep |VB.
LW    Cep |Depth of Min II 0.05m.
LZ    Cep |Min II 5.63. In the Table: P(Vr) [04627].
MN    Cep |Depth of Min II 0.08m?
MQ    Cep |Min II 15.7.
MT    Cep |Min II 15.5.
MX    Cep |SB (P = 16.03d) [08947].
MY    Cep |In the cluster NGC 7419. Emission OH, H2O.
MZ    Cep |In the region of the cluster NGC 7419.
NN    Cep |Min II 8.52.
NR    Cep |Min II 13.6; d = 0.025P?
NS    Cep |Depth of Min II 0.04m.
NW    Cep |Preceding component of a close VB. Min II 10.7.
NY    Cep |VB A (B 10.33m, 10", 190deg); d = 0.003P; SB2, e = 0.49;
NY    Cep |Delta(gamma) = gamma2 - gamma1 = 32 km/s  [07412].
OS    Cep |Very red.
OT    Cep |Min II 13.3.
OZ    Cep |Red.
PS    Cep |In the region of the cluster NGC 7380. SB2 (P = 2.09168d)
PS    Cep |[05479].
PV    Cep |In the dark cloud near the diffuse nebula and the cluster
PV    Cep |NGC 7023. At the apex of the bright variable fan nebula.
PW    Cep |In the region of the diffuse nebular and the cluster
PW    Cep |NGC 7023.
QZ    Cep |The map of surroundings given in [04015] for BV 323 is in
QZ    Cep |reality the map for BV 324 = QZ Cep. Min II 11.9.
V0338 Cep |Min II 9.52.
V0342 Cep |B - V = +3.6.
V0344 Cep |B - V = +4.4.
V0345 Cep |B - V = +5.0.
V0346 Cep |B - V = +4.6.
V0347 Cep |B - V = +4.5.
V0351 Cep |VB A (B 13m, 20", 135deg). P var. Max = 2430615.57 +
V0351 Cep |2.80511d*E (JD2429160 - 34300); Max = 2435749.12 +
V0351 Cep |12.80556d*E (JD2435310 - 40885) [02830]. Since
V0351 Cep |JD2442020 - see Table.
V0421 Cep |SB, Porb1 = 5.4136d, Porb2 = 225.44d.
V0447 Cep |The variability may be due to the fainter (B) component.
V0448 Cep |SB, Porb = 7.7320d.
V0453 Cep |SB, Porb = 54.723d.
V0454 Cep |SB, Porb = 5.6556d.
V0711 Cep |Variability refers to combined brightness of two nearly equal
V0711 Cep |components at 5" separation.
bet   Cep |VB A (A 6m, 0.204", 47.2deg, 1977.9; B 7.84m, A2V, 13.6",
bet   Cep |250deg). SB1 (Porb = 10.893d) [06486]. P var.
bet   Cep |Max(Vr) = 2417359.715 + 0.1904795d*E (JD2415750 - 22000);
bet   Cep |Max(Vr) = 2422203.790 + 0.1904844d*E +
bet   Cep |2.9440d*10**(-11)*E**2 + 3.2671d*10**(-17)*E**3
bet   Cep |(JD2422000 - 42630) [00177]. Elements given in the Table
bet   Cep |satisfy observations in 1967 - 69.
del   Cep |VB A (B 13.0m, 20.0", 285deg; C 6.10m - 6.37m, B7IV,
del   Cep |41.0", 191deg. P var. Max = 2393659.856 + 5.366438d*E
del   Cep |(JD2372200 - 96900); Max = 2413960.73 + 5.366386d*E
del   Cep |(JD2396900 - 2414050); since JD2414050 - see Table.
del   Cep |All observations in the interval JD2373090 - 45000 are
del   Cep |well represented also by the elements with a square term:
del   Cep |Max = 2442756.490 + 5.366270d*E - 7d*6*10**(-9)*E**2
del   Cep |[08632].
eps   Cep |VB A (B 9.5m, 127.8", 15deg, 1918).
eps   Cep |Multiperiodicity: P2 = 0.068073d
eps   Cep |(A2/2 = 0.0061m), P3 = 0.011823d? (A3/2 = 0.0022m);
eps   Cep |A1/2 = 0.0079m.
zet   Cep |Radial velocity varies.
mu    Cep |VB A (B 12.3m, 19.4", 262deg; C 12.7m, 41", 299deg).
mu    Cep |There is also the cycle with 4400d duration [08957].
W     Cet |S5.5/2e.
RR    Cet |[Fe/H] = -1.26. P var. During JD2417500 - 28820
RR    Cet |Max = 2417501.444 + 0.55302577d*E; since JD2433180 - see
RR    Cet |Table. According to [08726], the graph of O - C deviations
RR    Cet |from the elements given in [03506] is approximately
RR    Cet |sinusoidal, with Pi = 2600d and the amplitude 0.025d.
RU    Cet |(k - b)2 = 0.01. Delta(m) var? P var [02455]. Max =
RU    Cet |2426964.019 + 0.5863003d*E (JD2426500 - 28430)
RU    Cet |[00181]; Max = 2434143.056 + 0.5862676d*E
RU    Cet |(JD2433100 - 35820) [02431]; since JD2435820 - see Table.
RV    Cet |Delta(S) = 9.
RW    Cet |Min II 10.5. P var. During JD2426500 - 41000
RW    Cet |Max = 2426585.503 + 0.9751814d*E [00001]; since
RW    Cet |JD2441000 - see Table.
RX    Cet |Delta(S) = 5. P var. Before JD2428500 Max =
RX    Cet |2425938.271 + 0.5737100d*E [03506]; since
RX    Cet |JD2430000 - see Table.
RZ    Cet |Delta(S) = 6.7. P var. During JD2426585 - 28630
RZ    Cet |Max = 2426585.448 + 0.510633d*E [03506]; current
RZ    Cet |elements - see Table.
SS    Cet |d = 0.025P. P var. Min = 2429321.250 + 2.9739509d*E
SS    Cet |(JD2427340 - 30700) [02419]; Min = 2430698.160 +
SS    Cet |2.973992d*E (JD2429300 - 36650) [03115];
SS    Cet |since JD2440000 - see Table.
SV    Cet |Min II 14.9.
TT    Cet |Min II 11.1.
TU    Cet |D = 0.043P. Min II 10.9. Min II - Min I = 0.478P.
TU    Cet |According to [03564], the spectrum is K2.
TV    Cet |Min II 9.10. DII = 0.03P. Min II - Min I = 0.494P.
TW    Cet |Min II 11.14. P var. Min I = 2430965.595 +
TW    Cet |0.316852d*E (JD2427650 - 31000) [00192]; Min I =
TW    Cet |2433611.3121 + 0.316846d*E (JD2433530 - 615)
TW    Cet |[00001]; since JD2440000 - see Table.
TX    Cet |B - V: +0.34, +0.37. Min II 11.12.
TY    Cet |Min II 12.1.
UU    Cet |(k - b)2 = 0.08. P var. Blazhko effect?
UV    Cet |VB B (A 12.45m, dM5.5e; a = 2.1", P = 25a).
VV    Cet |Min II 11.0. EB type is also possible. RR type with twice
VV    Cet |shorter period is not excluded.
VX    Cet |d = 0.026P.
VY    Cet |Min II 11.70.
VZ    Cet |ADS 1778 B (B 0.61", 122deg; A = omicron Cet).
VZ    Cet |Small variations are also observed on the time scale of
VZ    Cet |several hours, with superimposed 10 - 15 minute variations
VZ    Cet |and rare flares of approximately 2 minute duration
VZ    Cet |[06492]. A possible white dwarf with an accretion
VZ    Cet |disc [08926].
WW    Cet |VR var (P = 0.160d) [04712].
WW    Cet |Rapid oscillations (~10 min) of brightness are observed
WW    Cet |[04709].
WZ    Cet |Min II 11.0.
XY    Cet |d = 0.02P. Min II 9.34.
YY    Cet |Min II 9.2.
ZZ    Cet |4 stable oscillations are observed simultaneously:
ZZ    Cet |P1 = 213.132605s, P2 = 212.768427s, P3 = 274.250814s,
ZZ    Cet |P4 = 274.774562s.
AA    Cet |ADS 1581 A (B 7.7m vis, SB 2, F5, 8.5", 304deg).
AA    Cet |Min II 6.7:. dII = 0.065P.
AB    Cet |ADS 1849 A (B 9.30m, 12", 293deg). SB? (VR var,
AB    Cet |P = 2.997814d). The period of magnetic variations is
AB    Cet |15.9d [08932].
AD    Cet |ADS 180 A (B 10m, 3", 4deg).
CL    Cet |Type ELL: is also possible.
EE    Cet |The variability may be due to the fainter (B) component.
EL    Cet |SB2.
del   Cet |Nonlinear term: +2.20d*10**(-11)*E**2.
omi   Cet |ADS 1778 A (B = VZ Cet, 0.61", 122deg). Maser
omi   Cet |SiO, OH, H2O.
S     Cha |VB A (B 9.29m, 23", 134deg).
T     Cha |Occasionally quasiperiodic light changes are observed with
T     Cha |periods 3.2323d, 3.4375d, 4.1800d, 3.2436d operating
T     Cha |during 6 - 26 cycles. IR excess.
Z     Cha |VB A (B 5.6"). Eclipses: Min =
Z     Cha |2440264.68232 + 0.0744992195d*E + 7.88d*10**(-13)*E**2
Z     Cha |[08938]. D = 0.065P; d = 0.026P. Depth of Min:
Z     Cha |1.73m - 2.11m B before the eclipse; 1.38m - 1.97m B after
Z     Cha |the eclipse. Periodic variations during Min light [07000].
Z     Cha |Variations with P = 27.7s during a supermaximum [08049].
RS    Cha |EA/DM. Min II 6.53. One of the components is a pulsating
RS    Cha |variable of DSCT type. P is in the range from 0.074d
RS    Cha |to 0.097d [08403]. Delta(M) = 0.01m - 0.03m in the combined
RS    Cha |light.
RW    Cha |Min II 14.6.
RY    Cha |Min II 14.0.
RZ    Cha |Min II 8.8. DII = 0.11P.
SY    Cha |Quasiperiodic variations were observed. (P = 6.2d [04305],
SY    Cha |P = 7.6d [08946]).
TW    Cha |Quasiperiodic variations (P = 8.68d [04462]).
VW    Cha |IR excess.
VZ    Cha |Quasiperiodic variations (P = 7.27d).
YZ    Cha |Delta(m) (Min II) = 0.4m.
CG    Cha |Min II 14.4.
CH    Cha |Min II 15.1.
CX    Cha |Min II 15.5. Uncertain elements.
CY    Cha |Min II 14.0.
CZ    Cha |Min II 14.6.
DD    Cha |Min II 14.7.
DG    Cha |Min II 14.5.
zet   Cha |SB.
S     Cir |Min II 10.9.
T     Cir |Min II 9.4.
U     Cir |P var. Before JD2417000 Max = 2412560 + 151d*E.
V     Cir |Min II 11.0. According to [00210], varies in the range
V     Cir |10.8m - 13.0m pg.
W     Cir |Found in Lupus, in 4deg to the north from the position
W     Cir |published by the discoverer [00211].
TW    Cir |Min II 13.3.
UY    Cir |Red.
UZ    Cir |Epoch of main Max is given. Resembles R Cen.
UZ    Cir |Max I - Max II = 160d.
VX    Cir |P var. Before JD2418000 Max = 2414360 + 427d*E.
AQ    Cir |Possibly EW type with twice longer period.
AR    Cir |The magnitude in Min light possibly corresponds to an
AR    Cir |unresolved companion.
AT    Cir |d = 0.02d:.
AX    Cir |SB. VB? (6.5m; 6.5m; 0.5", 143deg, 1913).
BD    Cir |Min II 9.5.
BF    Cir |Min II 8.9.
BG    Cir |Min II 10.3.
BN    Cir |Deep Min II. Twice shorter period is not excluded.
BR    Cir |Cir X-1. According to [08951], the object does not coincide
BR    Cir |with the star (B = 22.5m) labelled as L in the chart in
BR    Cir |[02911] but is situated in ~1" to the south of it and has
BR    Cir |M > 23.5m on IIIa-J plates. Gradual increase of X-ray
BR    Cir |intensity is periodically stopped by an abrupt intensity
BR    Cir |fall. The moments of such transitions T are represented by
BR    Cir |the elements T = 2443292.118 + 16.595d*E [02926]. The X-ray
BR    Cir |intensity falls are accompanied by IR and radio bursts.
BR    Cir |Vr (e alpha) = +250 km/s. In 25' from the supernova
BR    Cir |remnant G 321.9-0.3.
tet   Cir |VB (6.2m, 6.2m, 0.1", 96deg).
T     Col |SiO maser.
U     Col |Min II 10.5.
Y     Col |V2 (NGC 1851).
Z     Col |V1 (NGC 1851).
RS    Col |Min II 9.97. dII = 0.021P.
RY    Col |(k - b)2 = 0.10. P var; nonlinear term: -3.38*10**(9)E**2.
RZ    Col |Min II 11.20.
VW    Col |Variability may be due to component B.
TV    Col |2A 0526 - 328. VB A (B 15.79m, 10", 330deg). Epoch of Max
TV    Col |of short-term photometric variations is given. The
TV    Col |following elements describe, respectively, moments of Max
TV    Col |Vr for Balmer lines and moments of Max for the
TV    Col |comparatively long-term photometric variations which are
TV    Col |due to the beat phenomenon for the photometric and
TV    Col |spectral periods: Max Vr = 2444227.631 + 0.228600d*E;
TV    Col |Max = 2444191.5 + 4.024d*E. Flickering up to 0.15m B and
TV    Col |flares up to 0.3m U are also observed [08960].
R     Com |OH emission.
S     Com |Delta(S) = 8.
T     Com |OH, H2O emission.
U     Com |Delta(S) = 5.
V     Com |P var. Max = 2424518.219 + 0.46913844d*E
V     Com |(JD2420900 - 26900) [00218]; since JD2438100 - see Table.
V     Com |Delta(S) = 8.
W     Com |Radio source ON 231.
X     Com |Z = 0.092. Spectrum description [07415,08966].
Y     Com |In the region of the globular cluster M 53 (NGC 5024).
Z     Com |In the region of the globular cluster M 53 (NGC 5024).
RR    Com |In the region of the globular cluster M 53 (NGC 5024).
RS    Com |In the region of the globular cluster NGC 5053.
RT    Com |In the region of the globular cluster NGC 5053. A var;
RT    Com |P var. Max = 2423113.496 + 0.5651925d*E (JD2422700 -
RT    Com |26450) [00222]; since JD2438535 - see Table.
RU    Com |In the region of the globular cluster M 53 (NGC 5024).
RV    Com |In the region of the globular cluster M 53 (NGC 5024).
RW    Com |In the region of the Comae Berenices cluster. dI = 0.04P;
RW    Com |Min II 11.56. P var.
RW    Com |Min I = 2433040.406 + 0.23734705d*E (JD2419680 - 34550)
RW    Com |[00185]; since JD2439600 - see Table.
RY    Com |P var. Max = 2425007.450 + 0.46894835d*E (JD2425000 -
RY    Com |27500) [03506]; Max = 2432674.390 + 0.4689397d*E
RY    Com |(JD2432600 - 38110) [03415]; since JD2438100 - see Table.
RY    Com |(k - b)2 = 0.07.
RZ    Com |Possible member of the Comae Berenices cluster. Min II
RZ    Com |11.09; dI = 0.043P, dII = 0.039P. P var.
RZ    Com |Min I = 2433396.737 + 0.33850556d*E (JD2425000 - 33300)
RZ    Com |[00226]; since JD2433300 - see Table.
RZ    Com |Shape of the light curve varies.
SS    Com |Min II 11.9.
ST    Com |Delta(S) = 10.
SX    Com |In the region of the globular cluster NGC 4147.
SZ    Com |In the region of the globular cluster NGC 4147.
TU    Com |Shape of the light curve, A and P vary. Mean elements
TU    Com |are given in the Table. Possible period of Blazhko effect
TU    Com |is 75d [03584]. [Fe/H] = -1.43.
UU    Com |Member of the Comae Berenices cluster. Light variations
UU    Com |are due to rotation and pulsations of the star. Rotational
UU    Com |period is 2.1953d or 1.0256d or 0.9178d. Period of
UU    Com |pulsations is 0.0227d (A ~0.01m). According to [07985]
UU    Com |there are two periods of pulsations: P1 = 0.0274d and
UU    Com |P2 = 0.0209d
UU    Com |(P2/P1 = 0.76).
UV    Com |[Fe/H] = -1.44.
UW    Com |[Fe/H] = -1.22.
UX    Com |Min II 10.13. P var; nonlinear term: -3.75d*10**(-8)*E**2.
UY    Com |[Fe/H] = -1.51.
UZ    Com |[Fe/H] = -1.44.
VV    Com |[Fe/H] = -1.53.
VW    Com |VB (12.00m, dM 3.5e; 12.3m, dM 4e, 3.0", 23deg, 1945).
VW    Com |Range of total brightness variation
VW    Com |is given. According to [08363] the component B is
VW    Com |variable. However both components may be variables.
VY    Com |Min II 14.5.
AI    Com |Member of the Comae Berenices cluster. VB A (B 6.63m,
AI    Com |145", 251deg). Pulsations are possible: P = 0.052d
AI    Com |(A = 0.02m) [08975].
AL    Com |Within 8' to the south-east from the nucleus of M 88
AL    Com |(NGC 4501) galaxy.
AQ    Com |Min II 15.7.
BM    Com |Min II 13.8.
BS    Com |P var. Max = 2434453.31 + 0.36341d*E (JD2434130 - 35230);
BS    Com |since JD2435590 - see Table. Shape of the light curve
BS    Com |varies.
BZ    Com |[Fe/H] = -1.21.
CC    Com |In the region of the Comae Berenices cluster. Min II
CC    Com |12.09; dI = 0.03P.
CD    Com |[Fe/H] = -1.78.
CF    Com |Shape of the light curve varies.
CG    Com |[Fe/H] = -1.06.
CI    Com |RRC?
CK    Com |P var. Max = 2437370.71 + 0.6940159d*E (JD2437370 - 40130);
CK    Com |Max = 2441630.35 + 0.6939080d*E (JD2440130 - 41630);
CK    Com |since JD2441630 - see Table. Blazhko effect.
CK    Com |[Fe/H] = -1.68.
CL    Com |[Fe/H] = -1.00.
CN    Com |Min II 13.5.
CP    Com |[Fe/H] = -1.19.
CT    Com |In the region of the Comae Berenices cluster.
CV    Com |In the region of the Comae Berenices cluster.
CX    Com |In the region of the Comae Berenices cluster. Not member
CX    Com |of the cluster.
DD    Com |Min II 14.90.
DG    Com |Min II 14.6.
DL    Com |P var?
DR    Com |EW? P = 0.45184d?
DS    Com |[Fe/H] = -1.32.
DT    Com |[Fe/H] = -1.60.
DU    Com |[Fe/H] = -1.45.
DV    Com |[Fe/H] = -1.57.
DW    Com |[Fe/H] = -1.53.
EE    Com |P = 0.539533d also satisfies observations. [Fe/H] = -1.64.
EF    Com |[Fe/H] = -1.90.
EG    Com |[Fe/H] = -1.29.
EI    Com |[Fe/H] = -1.68.
EL    Com |P = 0.52362d also satisfies observations.
EM    Com |[Fe/H] = -1.64.
EN    Com |[Fe/H] = -1.19.
EO    Com |[Fe/H] = -1.51.
EP    Com |[Fe/H] = -0.98.
EQ    Com |Min II 15.3.
ER    Com |[Fe/H] = -1.51.
ES    Com |[Fe/H] = -2.02.
EW    Com |[Fe/H] = -1.77.
EX    Com |P = 0.558359d? [Fe/H] = -1.48.
EY    Com |Min II 18.0.
EZ    Com |P = 0.568349d? [Fe/H] = -1.16.
FG    Com |P = 0.3098d also satisfies observations.
FK    Com |Wide emission lines, Halpha and H, K CaII, of variable
FK    Com |intensity. Epoch of light minimum is given.
FM    Com |The member of the Comae Berenices cluster. Multiperiodicity.
FM    Com |Cycle of 0.0713d was observed also [08989].
FO    Com |In the region of the Comae Berenices cluster.
FP    Com |In the region of the Comae Berenices cluster. mu = 0.23",
FP    Com |P = 158deg. Red.
FZ    Com |P = 4.704864d?
GM    Com |In the region of the Comae Berenices cluster.
GN    Com |Member of the Comae Berenices cluster. P > 1d.
GO    Com |In the region of the Comae Berenices cluster.
GP    Com |mu = 0.38", p = 286deg. SB (Porb = 0.032306d).
GP    Com |Unique object G 61-29. Consists of two interacting white
GP    Com |dwarfs. The lower mass star, a helium white dwarf,
GP    Com |transfers mass to the higher mass star surrounded by an
GP    Com |accretion disk. Usually flares are being observed with an
GP    Com |amplitude about 0.2m V, 0.5m U lasting about 20 seconds
GP    Com |[07417,08991]. Sometimes periods of photometric activity
GP    Com |arise when amplitude of light variations reaches 0.6m V
GP    Com |and sharp passages from maxima to minima are being
GP    Com |observed; the duration of these minima reaches up to 0.14d
GP    Com |[07417]. When the star is most active, periodic light
GP    Com |oscillations appear with P = 105 seconds and amplitude
GP    Com |0.05m - 0.10m V [07062].
GQ    Com |Z = 0.165. Emission H, [OIII]. Irregular light variations.
GQ    Com |<B - V> = +0.16.
GT    Com |Minor planet (679) Pax.
HH    Com |Epoch of Min in V system is given.
HI    Com |In the region of the Comae Berenices cluster.
HK    Com |In the region of the Comae Berenices cluster.
HM    Com |In the region of the Comae Berenices cluster.
HN    Com |In the region of the Comae Berenices cluster.
HO    Com |In the region of the Comae Berenices cluster.
HP    Com |In the region of the Comae Berenices cluster.
HQ    Com |In the region of the Comae Berenices cluster.
HR    Com |In the region of the Comae Berenices cluster.
HS    Com |In the region of the Comae Berenices cluster.
HT    Com |In the region of the Comae Berenices cluster.
HU    Com |In the region of the Comae Berenices cluster.
HV    Com |In the region of the Comae Berenices cluster.
HW    Com |In the region of the Comae Berenices cluster.
R     CrA |In the head of the bright cometary nebula NGC 6729.
R     CrA |IR excess.
S     CrA |VB A (B 13.5m, 1", 137deg). IR excess.
T     CrA |In the bright cometary nebula NGC 6729. IR excess.
V     CrA |Quasiperiodic variations (P ~75d, Delta(V) ~ 0.2m - 0.9m).
V     CrA |IR excess.
RS    CrA |sp of two close stars; each of them or both may be
RS    CrA |identified with CoD -39deg 13082.
RW    CrA |Min II 9.4.
SS    CrA |V1 (NGC 6541).
SV    CrA |The period may be twice shorter.
TY    CrA |VB A (B 13.3m, 4", 138deg; C 58", 24deg).
TY    CrA |In the bright nebula NGC 6726/27. P = 1.92d is not
TY    CrA |excluded, in that case Min II = Min I. On the basis of
TY    CrA |visual observations 8.7 - 12.4 v (presumably "spurious
TY    CrA |variability" due to the difficulties of estimates over
TY    CrA |the bright background of the nebula), and the star
TY    CrA |was classified as INSA.
TZ    CrA |Min II 9.72.
UU    CrA |Min II 11.0.
UX    CrA |The period may be twice shorter.
UY    CrA |P var?
VV    CrA |In the region of the bright nebula NGC 6729. IR excess.
AF    CrA |P var. Before JD2418060 Max = 2413710 + 483d*E; since
AF    CrA |JD2418060 - see Table.
AL    CrA |B - V: +0.65, +1.30. [A/H] = -0.2.
AN    CrA |P var. Nonlinear term: -0.006d*10**(-6)*E**2.
AU    CrA |P var. Nonlinear term: -0.026d*10**(-6)*E**2.
AY    CrA |Min II 15.2.
BG    CrA |Min II 15.1.
BH    CrA |P var. Nonlinear term: -0.023d*10**(-6)*E**2.
CM    CrA |P var. Nonlinear term: -0.007d*10**(-6)*E**2.
CR    CrA |Min II 15.7.
CS    CrA |Min II 15.2.
CY    CrA |P var. Nonlinear term: -0.002d*10**(-6)*E**2.
DG    CrA |In the region of the bright nebula NGC 6729. IR excess.
DL    CrA |Min II 13.6.
DN    CrA |P var. Nonlinear term: +0.006d*10**(-6)*E**2.
DZ    CrA |d = 0.02P.
EE    CrA |<mpg> var, 13.5m - 15.5m, P2 = 3000d - 5000d
EE    CrA |Delta(m) (P1 = 167d) ~1.5m.
EK    CrA |P var. Before JD2422600 Max = 2411870 + 421d*E.
FF    CrA |Before JD2423000 Max = 2411530 + 140.2d*E.
FK    CrA |Min II 14.5.
FS    CrA |Min II 14.5.
FW    CrA |Before JD2416600 Max = 2411190 + 112.2d*E.
GS    CrA |Before JD2422600 Max = 2414070 + 284d*E.
IT    CrA |Min II 13.6.
KM    CrA |The chart in [06286] is wrong.
KQ    CrA |[A/H] = -0.7. B - V: +0.76, +1.23.
KT    CrA |Red.
LU    CrA |P = 182d is possible.
MS    CrA |Yellow.
MT    CrA |Min II 13.1.
NO    CrA |Reddish.
QR    CrA |Reddish.
V0347 CrA |B - V: +0.82, +1.17.
V0350 CrA |Min II 13.4.
V0385 CrA |The period may be spurious.
V0413 CrA |(k - b)2 = 0.11.
V0428 CrA |The period may be twice shorter.
V0449 CrA |[A/H] = -0.3.
V0454 CrA |Min II 10.5.
V0455 CrA |d = 0.05P. Min II 13.7.
V0457 CrA |Epoch of Min is given. EW type is also possible, in that
V0457 CrA |case the value of P should be doubled.
V0465 CrA |Min II 14.2.
V0467 CrA |P var?
V0471 CrA |Min II 13.3.
V0478 CrA |Sometimes a cycle 60d - 70d.
V0480 CrA |Min II 13.9.
V0490 CrA |P var? The elements represent the observations of 1944.
V0493 CrA |P var?
V0501 CrA |Min II 13.4. Twice shorter period is possible.
V0503 CrA |d = 0.03P.
V0511 CrA |Twice longer period is possible.
V0512 CrA |P var?
V0513 CrA |Min II 13.2.
V0514 CrA |Min II 14.0.
V0527 CrA |P var.
V0535 CrA |P var.
V0541 CrA |P var?
V0545 CrA |VB. Combined brightness with a faint companion is given.
V0553 CrA |P var?
V0566 CrA |Min II 12.7.
V0568 CrA |Sometimes a cycle 60d - 80d.
V0569 CrA |Min II 13.1. EB type is possible.
V0571 CrA |Min II 14.7.
V0572 CrA |Min II 14.0.
V0577 CrA |Min II 13.2. RR type with twice shorter period is possible.
V0578 CrA |RV type with P = 118d is possible.
V0580 CrA |Min II 14.4.
V0595 CrA |P var.
V0601 CrA |Epoch of min is given.
V0603 CrA |Slightly noticeable Min II at the phase 0.5P.
V0604 CrA |d = 0.03P.
V0607 CrA |Min II 14.3.
V0612 CrA |d = 0.03P.
V0615 CrA |P var?
V0622 CrA |Sometimes 55d - 60d cycles.
V0633 CrA |P var.
V0634 CrA |Min II 13.9.
V0648 CrA |Min II is felt at the phase 0.5P.
V0659 CrA |P = 189.4d is possible.
V0667 CrA |In the region of the bright cometary nebula NGC 6729.
V0667 CrA |The spectral type is earlier than K.
V0676 CrA |RR type is possible.
V0686 CrA |Max I 5.34, Min I 5.41, Max II 5.35, Min II 5.40 [08970].
V0691 CrA |4U 1822-37. Emissions CIII/NIII lambda 4640 - 50,
V0691 CrA |He II lambda 4686, CIV lambda 1550 etc.
V0692 CrA |P = 0.83d is possible.
eps   CrA |Min II 4.95.
R     CrB |IR excess.
S     CrB |OH, H2O, SiO maser.
T     CrB |VB? A (B <= 12m, 0.2"). SB (P = 227.6d).
T     CrB |The spectral period is present in the photometric data of
T     CrB |1891 - 1917 and 1960 - 1971 [08978]. The epoch of the first
T     CrB |outburst JD2402734 (1866). Two smaller outbursts were
T     CrB |observed in UV light, JD2438030 (1963) and 2442543
T     CrB |(1975) [08979].
U     CrB |Min II 7.72. P var.
RR    CrB |P2 = 377d. Delta(m) (P1) ~0.5m, Delta(m) (P2) ~0.6m.
RS    CrB |P2 = 69.5d [01100]. Main period oscillation: 9.1m - 11.6m.
RT    CrB |Nonlinear term: +2.01d*10**(-8)*E**2. Min II 10.52 (var).
RT    CrB |DII = 0.09P.
RV    CrB |P var. Max = 2428285.608 + 0.3316217d*E (JD2428285 - 31610);
RV    CrB |Max = 2431705.349 + 0.3317313d*E
RV    CrB |(JD2431705 - 32954); Max = 2433030.572 + 0.331705d*E
RV    CrB |(JD2433030 - 36814) [05496]; Max =
RV    CrB |2440001.453 + 0.331569d*E (1967 - 1971) [06237];
RV    CrB |Max = 2441451.413 + 0.331619d*E (1972 - 1974)
RV    CrB |[07032]. The Table gives current elements. On
RV    CrB |the period changes see also [03506]. Blazhko effect?
RW    CrB |d = 0.028P. Min II 10.29.
TW    CrB |Min II 11.0.
TZ    CrB |ADS 9979 A (B 6.72m, GIV, 6.6", 233deg, 1980).
TZ    CrB |SB2 (P = 1.139789d).
TZ    CrB |Epoch of Min is given. The variation presented in the
TZ    CrB |Table is superimposed by a second one, with the same
TZ    CrB |amplitude and P = 0.1d. The amplitude is given
TZ    CrB |for the combined light of ADS 9979 A and B, the
TZ    CrB |mean magnitude is for ADS 9979 A.
UU    CrB |During JD2444381.73 - .76 a slow flare was observed, with
UU    CrB |maximal amplitude 0.30m in the IK band and 0.18m in the
UU    CrB |U band.
AL    CrB |Spotted rotating G-type giant.
alf   CrB |lambda eff = 7230 A: DI = 0.034P, DII = 0.018P,
alf   CrB |Min II - Min I = 0.66P, depth of Min I 0.10m, Min II
alf   CrB |0.025m.
bet   CrB |VB A (B ~ 5m - 6m, 0.2",  ~130deg, 1978). SB (P = 3833.7d).
bet   CrB |Magnetic field var, P = 18.487d. The epoch of Min light
bet   CrB |is given.
gam   CrB |ADS 9757 (4.2m, 5.6m; A = 0.74", P = 91.0a).
U     Crv |VB A (B 13.5m, 0.4' p).
W     Crv |Min II 11.86. The light curve is asymmetrical, the maxima
W     Crv |differ in hight by 0.10m.
Y     Crv |Min II 11.7. RRC type with twice shorter period
Y     Crv |is possible.
Z     Crv |d = 0.06P.
RV    Crv |Elements do
RV    Crv |not satisfy some of the published moments of Min.
RZ    Crv |Min II 13.9.
SX    Crv |Min II 9.23. The shape of the light curve varies. Depth of
SX    Crv |Min I 0.20m, depth of Min II 0.18m. In 1972 the system
SX    Crv |became fainter than in 1971 by 0.06m.
TY    Crv |SB2.
R     Crt |Periods of light constancy which last up to 250d occur
R     Crt |every two or there thousand days. OH, H2O maser.
S     Crt |H2O maser.
T     Crt |Mean light var, P2 = 1006d.
V     Crt |Min II 10.1; Min II - Min I = 0.57P.
W     Crt |(k - b)2 = +0.21.
X     Crt |(k - b)2 = +0.02.
Z     Crt |d = 0.016P.
RR    Crt |P = 293d or 146d is possible.
RV    Crt |Min II 9.4:.
SU    Crt |[Fe/H] > -0.3.
SV    Crt |ADS 8115 A (B 11.5m vis, 1", 220deg). SB2 (P = 5.90513d,
SV    Crt |apsidal motion, P ~700a). Epoch of Min I in B light is
SV    Crt |given. Depth of Min II is 0.015m. EuII and SrII in
SV    Crt |emission.
R     Cru |In the region of the open cluster NGC 4349.
T     Cru |In the region of the open cluster NGC 4349.
U     Cru |P var. Max = 2410143 + 351.4d*E (JD2410100 - 14100) [00237];
U     Cru |since JD2437600 - see Table.
W     Cru |Min II 9.3.
SU    Cru |[A/H] = -0.8.
SV    Cru |In the region  of the open cluster Ruprecht 97.
SV    Cru |Non-member of the cluster.
SW    Cru |VB A (B 14.0m, 12"). (k - b)2 = 0.27.
SY    Cru |d = 0.05P?
TU    Cru |Min II 11.5.
TW    Cru |Min II 12.85:.
TX    Cru |It is not excluded that actually P is much shorter,
TX    Cru |close to 1d, for instance.
TZ    Cru |P = 2.091140d?
UW    Cru |Min II 12.9; Min II - Min I = 0.536P.
UX    Cru |VB A (B 10"). Min II 12.4; Min I - Min II = 0.325P;
UX    Cru |DII = 0.025P.
VY    Cru |Min II 13.5.
VZ    Cru |P = 1.125810d?
WW    Cru |Min II 13.0.
WX    Cru |d = 0.040P. Light variability in maximum is noted.
WY    Cru |VB A. P = 9.013290d?
XX    Cru |P = 3.28566d?
XY    Cru |Min II 11.7.
XZ    Cru |P = 1.6495930d?
YY    Cru |Min II 13.0.
YZ    Cru |Min II 13.1.
ZZ    Cru |Min II 9.8.
AB    Cru |Min II 8.9.
AC    Cru |Min II 12.1.
AD    Cru |VB A (B 14.5m, 10", 270deg). P var. Max = 2434918.160 +
AD    Cru |6.39844d*E (JD2423800 - 35400) [02309];
AD    Cru |since JD2441000 - see Table.
AE    Cru |Depth of Min II 0.03m.
AF    Cru |According to [01122] Algol-type with the elements:
AF    Cru |Min I = 2424988.959 + 1.895669d*E, D = 0.06P.
AF    Cru |This conclusion must be checked. The star deserves careful
AF    Cru |investigation.
AG    Cru |The blue component is possible [09004].
AI    Cru |In the region
AI    Cru |of the open cluster NGC 4103. Min II 9.94.
AQ    Cru |Min II 13.8.
AT    Cru |Min II 12.6.
AW    Cru |Min II 13.9.
AY    Cru |Min II 11.2.
BB    Cru |Min II 14.0.
BC    Cru |Depth of Min II 0.03m.
BD    Cru |Depth of Min II 0.05m.
BF    Cru |Min II 12.3.
BH    Cru |Epoch of Min I is given in the Table. The light
BH    Cru |curve like the light curves of R Cen and R Nor
BH    Cru |has two maxima and two minima of different
BH    Cru |depths. Max I 7.6m (0.22P), Min II 8.0m (0.41P),
BH    Cru |Max II 7.2m (0.53P).
BI    Cru |Spectrum description [04949].
BK    Cru |In Coalsack region.
BM    Cru |In Coalsack region.
BP    Cru |3U 1223-62. A unique X-system. Consists of an X-pulsar
BP    Cru |with pulse period 698s [09018] moving on an excentric
BP    Cru |orbit (E = 0.47) around the ellipsoidal B2 supergiant with
BP    Cru |orbital period of 41.51d. Accretion of the stellar wind
BP    Cru |from the primary star on the pulsar increases during the
BP    Cru |periastron passage. Therefore large X-flares are observed
BP    Cru |with the elements: T (X Max) = 2433158.09 + 41.51d*E.
BP    Cru |Optical flares are possible.
BQ    Cru |B - V: +1.13, +0.88.
BS    Cru |In the open cluster NGC 4755.
BT    Cru |In the open cluster NGC 4755.
BU    Cru |In the open cluster NGC 4755.
BV    Cru |In the open cluster NGC 4755.
BW    Cru |In the open cluster NGC 4755.
DU    Cru |The identification with NSV 06012 (SIMBAD) is wrong.
bet   Cru |VB A (B 11.4m, 44.3", 322deg; C 7.5m, 372", 23deg).
bet   Cru |Interferometric binary. Multiple periods (the total V
bet   Cru |amplitudes of corresponding oscillations are indicated
bet   Cru |in brackets): P0 = 0.2365072d (0.034m), P1 = 0.160466d
bet   Cru |(0.029m), P2 = 0.121383d (0.01m), P02 = 0.249373d
bet   Cru |(0.016m), P13 = 0.24273d (0.024m), P24 = 0.23931d
bet   Cru |(0.028m), P03 = 0.16342d (0.016m), P14 = 0.16171d
bet   Cru |(0.029m).
tet 2 Cru |SB (P = 3.4380d). BCEPS, P > 1h? [08420].
lam   Cru |Type ELL with
lam   Cru |P = 0.7902d is possible. Amplitude and shape of
lam   Cru |the light curve vary. The secondary oscillation
lam   Cru |(A = 0.007m) with the elements Max = 2441779.034 +
lam   Cru |0.1793d*E is possible.
R     Cyg |VB A (B 9.3m, 91", 14deg). S4/6e - S8/6e.
T     Cyg |VB A (B 10.03m, 10.2", 122deg; C 12m, 13.6", 197deg).
U     Cyg |VB A (B 7.8m, 63.5", 51deg). P var. Max = 2406455 +
U     Cyg |461.57d*E (JD2404590 - 13900); Max = 2414827 +
U     Cyg |470.76d*E (JD2413900 - 19940); Max = 2421806 +
U     Cyg |455.95d*E (JD2419940 - 27380); Max = 2427848 +
U     Cyg |472.85d*E (JD2427380 - 35750); since JD2435750 - see Table.
W     Cyg |There is a second oscillation with P = 235.3d.
X     Cyg |P var. Max = 2410190.86 + 16.3841d*E (JD2410100 -
X     Cyg |23370) [09028]; since JD2417000 - see Table.
X     Cyg |There is a square term in the elements given in the Table:
X     Cyg |+1.01d*10**(-7)*E**2. [A/H] = 0.4.
Y     Cyg |Min II 7.75; E = 0.1458. Apsidal motion: P = 47.6 yr.
Y     Cyg |There are sinusoidal terms in the elements:
Y     Cyg |+0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E));
Y     Cyg |Min II = 2409454.9174 + 2.9963328d*E -
Y     Cyg |0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E)).
Z     Cyg |OH, H2O emission.
RR    Cyg |VB A (B 12.5m, 18.1", 58deg).
RS    Cyg |VB A (B 7.09m, 132", 355deg; C 9.3m, 56", 106deg).
RS    Cyg |Epoch of light minimum is given. The shape of the light
RS    Cyg |curve strongly varies. Double maxima are sometimes
RS    Cyg |observed (Min II at the phase 0.5P).
RU    Cyg |VB A (B 12.40m V, 10", 224deg; C 11.15m V, 19", 29deg).
RV    Cyg |VB A (B 10m, 142", 118deg).
RY    Cyg |In the region of the open cluster NGC 6883.
RZ    Cyg |The shape of the light curve strongly varies. Alternation
RZ    Cyg |of high and low maxima, as well as of shallow and
RZ    Cyg |deep minima is observed, as a rule: 9.8m <= Max <= 12.0m.
RZ    Cyg |11.8m <= Min <= 14.1m.
SS    Cyg |SB2 (P = 0.27512995d [08285]).
SS    Cyg |During maxima of brightness there are oscillations of
SS    Cyg |light and X-ray flux with amplitudes about 0.002m V
SS    Cyg |and periods changing between 7.29s and 10.90s [06102,
SS    Cyg |09032].
SU    Cyg |P var. Max = 2421278.503 + 3.845507d*E (JD2414250 -
SU    Cyg |29000) [01559]; Max = 2433095.944 + 3.845664d*E
SU    Cyg |(JD2429000 - 33150) [00921]; since JD2434500 - see Table.
SV    Cyg |VB A (B 9.5m V, 145", 140deg).
SW    Cyg |Min II 9.30; d(V) = 0.018P; d(U) = 0.00P. P var. Min I =
SW    Cyg |2414782.448 + 4.572937d*E (JD2411340 - 16450);
SW    Cyg |Min I  = 2418440.758 + 4.5727923d*E (JD2417060 -
SW    Cyg |19740) [00063]; Min I = 2421504.489 + 4.572729d*E
SW    Cyg |(JD2421470 - 24970); Min I = 2425185.550 + 4.5728386d*E
SW    Cyg |(JD2424960 - 29500); Min I = 2433160.669 + 4.5729841d*E
SW    Cyg |(JD2433000 - 36800) [09085]; Min I = 2438584.3081 +
SW    Cyg |4.57311736d*E (JD2438600 - 40560) [09085];
SW    Cyg |since JD2441160 - see Table.
SY    Cyg |d = 0.040P. Possible depth
SY    Cyg |of Min II 0.03m.
SY    Cyg |P var. Min I = 2411659.568 + 6.00584d*E (JD2411600 -
SY    Cyg |17100); Min I = 2420001.571 + 6.005716d*E
SY    Cyg |(JD2418760 - 20760) [01961];
SY    Cyg |Min I = 2437069.254 + 6.005626d*E
SY    Cyg |(JD2432800 - 37070) [05416].
SY    Cyg |Mean elements given in the Table represent epochs of
SY    Cyg |Min I in the interval JD2414400 - 37070 up to +- 0.07d.
SY    Cyg |According to [04248] the apsidal motion with the period ~46
SY    Cyg |years is possible.
SZ    Cyg |[A/H] = 0.5. P var [02392].
SZ    Cyg |Mean elements given in the
SZ    Cyg |Table represent epochs of Max up to  +- 0.5d. According
SZ    Cyg |to [09029] "the O - C diagram has a sinusoidal structure
SZ    Cyg |as is to be expected for a member of a binary system"
SZ    Cyg |with P orb = 65 years.
TT    Cyg |VB A (B 10.8m V, 70", 213deg; C 11.1m V, 83", 49deg;
TT    Cyg |D 10.7m V, 94", 268deg).
TV    Cyg |According to [03663] - spectrum G0.
TX    Cyg |[A/H] = -0.2. P var. Max = 2436793.138 + 14.708157d*E
TX    Cyg |(JD2415000 - 37000); since JD2436700 - see Table.
UU    Cyg |VB A (B 10.7m V, 3.6", 351deg).
UV    Cyg |VB A (B 10.8m V, 0.9", 79deg).
UW    Cyg |P var. Min I = 2419624.501 + 3.450797d*E (JD2410000 -
UW    Cyg |20750) [00526]; Min I = 2419624.501 + 3.450752d*E
UW    Cyg |(JD2419620 - 33000); Min I = 2433848.508 + 3.450740d*E
UW    Cyg |(JD2430000 - 41800); since JD2441800 -
UW    Cyg |see Table. Possible depth of Min II 0.05m.
UX    Cyg |P var. Max = 2432444 + 560.3d*E (JD2415670 - 32450);
UX    Cyg |Max = 2439352 + 578.0d*E (JD2432450 - 40500);
UX    Cyg |since JD2437600 - see Table. Sometimes rapid light
UX    Cyg |decreases on the ascending branch near Max are observed
UX    Cyg |[01563,01564]. H2O, OH, SiO maser.
UY    Cyg |Delta(S) = 3.8.
UZ    Cyg |VB A (B 10.8m, 28", 130deg). d = 0.032P; Min II 10.31.
VV    Cyg |Min II 13.2. P var? [03665].
VW    Cyg |d = 0.035P; Min II 10.31. P var. Min I = 2417377.123 +
VW    Cyg |8.4305260d*E (JD2415660 - 17400); Min I =
VW    Cyg |2430444.061 + 8.4302826d*E (JD2417400 - 30450);
VW    Cyg |Min I = 2441116.868 + 8.4303917d*E + 4.31d*10**(-8)*E**2
VW    Cyg |(JD2430450 - 41120) [07096]; since JD2440350 - see Table.
VX    Cyg |[A/H] = 0.2. P var. There is a square term in the
VX    Cyg |elemenmts +8.02d*10**(-7)*E**2.
VZ    Cyg |P var. Max = 2437103.945 + 4.8645598d*E(JD2416000 -
VZ    Cyg |41000); since JD2434000 - see Table.
WW    Cyg |d = 0.008P; Min II 10.16. P var [06144]. Mean elements:
WW    Cyg |Min I = 2416981.299 + 3.3176924d*E (JD2412000 - 31000)
WW    Cyg |[00063]; since JD2431000 - see Table.
WZ    Cyg |Min II 10.9.
XX    Cyg |[Fe/H] = -0.49. P var. Max = 2430671.1010 +
XX    Cyg |0.134865026*E(2416560 - 30000); since JD2430000 - see
XX    Cyg |Table.
XZ    Cyg |[Fe/H] = -1.2. P var. Max = 2417201.241 + 0.4665878*E -
XZ    Cyg |0.000107d*10**(-6)*E**2 (JD2414000 - 35000) [02550];
XZ    Cyg |Max = 2438562.796 + 0.466570d*E (JD2434000 - 39800);
XZ    Cyg |Max = 2440445.789 + 0.466497d*E (JD2439800 - 41000)
XZ    Cyg |[06237]; Max = 2441453.3856 + 0.4664731d*E
XZ    Cyg |(JD2441000 - 42500) [07424]; Max = 2443028.641 +
XZ    Cyg |0.466438d*E (JD2442500 - 43800) [09101]; Max =
XZ    Cyg |2444142.650 + 0.466649d*E (JD2443800 - 44200)
XZ    Cyg |[09102]; since JD2444100 - see Table.
XZ    Cyg |Besides that the star has a strongly
XZ    Cyg |expressed Blazhko effect; the period of Blazhko effect
XZ    Cyg |varies, too [07424,07425]. 0.13P <= M - m <= 0.22P;
XZ    Cyg |0.90m <= A(B) <= 1.70m, 0.70m <= A(B) <= 1.30m;
XZ    Cyg |-0.05P < O - C < +0.05;
XZ    Cyg |Max A = 2417025.5 + 57.401d*E (JD2417000 - 38500);
XZ    Cyg |Max A = 2438881.7 + 58.387d*E (since JD2438500).[09103].
XZ    Cyg |After JD2444000
XZ    Cyg |Blazhko effect period probably decreased to 56.3d [09102].
ZZ    Cyg |VB A (B 12.63m, 8.5", 43deg.
ZZ    Cyg |Total brightness variation range
ZZ    Cyg |is given. Min II 10.78. P var. Min I = 2417442.419 +
ZZ    Cyg |0.6286185d*E (JD2415000 - 25800) [07427];
ZZ    Cyg |since JD2427950 - see Table.
AA    Cyg |S 6/3.
AC    Cyg |H2O maser.
AD    Cyg |S 5/5.
AE    Cyg |d = 0.039P; Depth of Min II 0.06m.
AF    Cyg |Light curve (1914 - 1956) [09104].
AF    Cyg |Two more independent oscillations are superimposed:
AF    Cyg |P2 = 175.8d, P3 = 941.2d.
AK    Cyg |VB A (B 11.06m, A7, 20", 85deg).
AV    Cyg |P var. Max = 2420451.9 + 87.48d*E (JD2418782 -
AV    Cyg |24823); Max = 2427936.3 + 89.73d*E (JD2426326 -
AV    Cyg |28745); Max = 2429440.9 + 87.69d*E (JD2428820 -
AV    Cyg |31260); Max = 2436413.8 + 89.63d*E (JD2434610 -
AV    Cyg |37130); since JD2437450 - see Table.
AV    Cyg |0.27P <= M - m <= 0.50P.
AX    Cyg |VB A (B 10.2m, 18", 52deg).
AY    Cyg |In the region of the open cluster Dolidze 2.
BB    Cyg |P var. Max = 2426360 + 265.7d*E (JD2414900 - 26700);
BB    Cyg |Max = 2433091 + 258.6d*E (JD2426700 - 35500); Max =
BB    Cyg |2438354 + 266.9d*E (JD35500 - 40200) [09106];
BB    Cyg |since JD2439200 - see Table.
BF    Cyg |P orb = 750d [05655].
BF    Cyg |Irregular light variations and sometimes observed
BF    Cyg |brightenings by 2m - 3m are superimposed by semiregular
BF    Cyg |oscillations with the cycle 755d [01039,08044].
BG    Cyg |P var. Max = 2421190 + 290.35d*E (JD2421150 - 29950);
BG    Cyg |Max = 2430546 + 307.3d*E (JD2429950 - 30850); Max =
BG    Cyg |2432872 + 289.5d*E (JD2430850 - 34920);
BG    Cyg |since JD2435100 - see Table.
BI    Cyg |VB A (B 9.4m, 126", 110deg).
BO    Cyg |D = 0.025P; Min II 12.0.
BR    Cyg |D = 0.020P; Min II 9.58.
BS    Cyg |SC 8/8. P var. Max = 2422655 + 420d*E (JD2422600 -
BS    Cyg |24750) [01161]; Max = 2425181 + 431.4d*E (JD2424750 -
BS    Cyg |26500) [01171]; since JD2437500 - see Table.
BY    Cyg |VB A (B 16m).
BZ    Cyg |[A/H] = 0.1. Double maximum.
CD    Cyg |[A/H] = 0.2. P var.
CD    Cyg |There is a square term in the elements:
CD    Cyg |+1.54d*10**(-6)*E**2.
CG    Cyg |VB A (B 11.8m, 1.3", 306deg; 1979.7).
CG    Cyg |10.10 <= Min II <= 10.44. P var.
CG    Cyg |Min I = 2422967.4248 + 0.63114347d*E
CG    Cyg |(JD2422900 - 38500); since JD2439000 - see Table. Combined
CG    Cyg |light range is given. Shape of the light curve varies
CG    Cyg |[08848].
CH    Cyg |Semiregular light variations with the mean cycle 97d;
CH    Cyg |mean brightness varies with the cycle ~4700d [01169].
CH    Cyg |There are also a cycle 725d [08849], rapid oscillations
CH    Cyg |(A <= 0.25m U) and flares [05350]. It is not excluded
CH    Cyg |that the system is an eclipsing one [06499].
CI    Cyg |d = 0.084P.
CI    Cyg |Depth of eclipses ~0.8m. The eclipses of B star are
CI    Cyg |observed. Usually there are light fluctuations near mean
CI    Cyg |brightness ( ~12.1m). The outbursts last some dozens
CI    Cyg |and hundreds days. Light curves [06155,08044,08850,
CI    Cyg |08851]. Emissions of H, He I, He II, [O III], and N III.
CM    Cyg |S 4/6.5e.
CU    Cyg |P var. Max = 2422643 + 223.8d*E (JD2422600 - 26500);
CU    Cyg |since JD2426500 - see Table.
CV    Cyg |dI = 0.06P; Min II 11.33. P var. Min I = 2424458.348 +
CV    Cyg |0.9834523d*E (JD2414300 - 24500); since JD2424450 - see
CV    Cyg |Table. Shape of the light curve and Min I depth vary.
CY    Cyg |SC 2/7.5.
CZ    Cyg |P var. Max = 2424500 + 284d*E (JD2424500 - 33600)
CZ    Cyg |[03122]; since JD2432700 - see Table.
DD    Cyg |P var. Max = 2425465 + 148.30d*E (JD2424800 - 39000)
DD    Cyg |[01149]; since JD2439000 - see Table.
DF    Cyg |P var [01177,06107]. Mean
DF    Cyg |brightness varies: Min = 2411292 + 780.2d*E [01571].
DG    Cyg |SiO maser?
DH    Cyg |OH emission?
DK    Cyg |dI = dII = 0.04P; Min II 10.90. P var.
DK    Cyg |Shape of the light curve and depth of Min II vary.
DL    Cyg |Min II 9.9.
DM    Cyg |P var. Max = 2425887.560 + 0.4198557d*E (JD2415200 -
DM    Cyg |25900) [03506]; Max = 2425887.5597 + 0.41985715d*E
DM    Cyg |(JD2425880 - 29250) [00522]; Max = 2433872.420 +
DM    Cyg |0.41985842d*E (JD2429250 - 37900) [03506]; Max =
DM    Cyg |2438677.708 + 0.4198619d*E (JD2438600 - 41250)
DM    Cyg |[07114]; since JD2441240 - see Table.
DM    Cyg |There is also Blazhko effect with the elements:
DM    Cyg |Max(O - C) = 2442978.97 + 26.01d*E [08853];
DM    Cyg |-0.01 d< = O - C <= +0.01d. Delta(S) = 0.
DQ    Cyg |P = 180d?
DT    Cyg |P var. Max = 2424305.651 + 2.49913d*E (JD2424300 -
DT    Cyg |28500) [01183]; Max = 2432792.893 + 2.49934d*E
DT    Cyg |(JD2430000 - 36000); since JD2436000 - see Table.
DV    Cyg |P var. Max = 2425476 + 146.7d*E (JD2415200 - 29200);
DV    Cyg |since JD2432800 - see Table.
DW    Cyg |P var. Max = 2427603 + 279.6d*E (JD2416700 - 33500);
DW    Cyg |since JD2433500 - see Table.
DX    Cyg |Min II 14.2; Min II - Min I = 0.515P; DI = 0.22P,
DX    Cyg |DII = 0.12P.
DY    Cyg |Slow oscillations are superimposed by rapid ones with
DY    Cyg |A = 0.3m [03662]. According to [03148] type EB?
DY    Cyg |Min = 2436659.531 + 0.6990d(:)*E (JD2436600 - 37000)
DY    Cyg |[03148].
EE    Cyg |Min II 14.5.
EF    Cyg |142d <= P <= 175d.
EH    Cyg |P var. Max = 2427608 + 276.90d*E (JD2416200 - 27610);
EH    Cyg |since JD2427800 - see Table.
EI    Cyg |Epoch of Max I is given; heights of Max I and Max II
EI    Cyg |differ strongly, the depths of Min I and Min II are almost
EI    Cyg |equal. Max I - Min I = 52d.
EK    Cyg |Observations are represented by the elements in the
EK    Cyg |interval JD2425200 - 37900 only.
EM    Cyg |Mean cycle varies in the range 19d - 33d [04248,09111].
EM    Cyg |Depth of eclipses 0.25m V; elements of eclipsing system
EM    Cyg |light variations: Min = 2437882.8595 + 0.29090950d*E -
EM    Cyg |21d*10**(-12)*E**2 [08854].
EM    Cyg |Sometimes there are light oscillations with periods
EM    Cyg |14.6s - 21.2s and an amplitude up to 0.4% [06102,09112].
EN    Cyg |d = 0.012P. P var. Min = 2425181.311 + 2.2148998d*E
EN    Cyg |(JD2424880 - 29600) [00332]; since JD2433500 - see Table.
ES    Cyg |P var. Max = 2425146 + 157d*E (JD2425000 - 29300)
ES    Cyg |[00332]; since JD2432800 - see Table.
EV    Cyg |P var. Max = 2427740 + 259.1d*E (JD2425100 - 29100);
EV    Cyg |since JD2433500 - see Table.
EV    Cyg |The position of the star in the chart in [00530] is wrong
EV    Cyg |[00782].
EZ    Cyg |P var? Shape of the light curve and the amplitude
EZ    Cyg |strongly vary; 0.40P < = M - m < = 0.48P.
FF    Cyg |S 5.5/6-e.
FG    Cyg |P var. Max = 2426955 + 456.0d*E (JD2416000 - 27000)
FG    Cyg |[00001]; Max = 2426955 + 458.8d*E (JD2426900 - 34300)
FG    Cyg |[03122]; since JD2439200 - see Table.
FM    Cyg |P var. Max = 2425313 + 274d*E (JD2425300 - 29200)
FM    Cyg |[00332]; since JD2429200 - see Table.
FN    Cyg |P var. Max = 2429137 + 314.6d*E (JD2416200 - 29200)
FN    Cyg |[00001]; since JD2432800 - see Table.
FO    Cyg |A var. P var. Max = 2425193 + 156.6d*E (JD2425000 -
FO    Cyg |29200) [00332]; since JD2432500 - see Table.
FR    Cyg |Min II 14.0; d = 0.03P.
FT    Cyg |P var. Max = 2425184 + 156.7d*E (JD2425100 - 29200)
FT    Cyg |[00332]. 83d <= P <= 187d (JD2432500 - 38000).
FY    Cyg |P var. Max = 2425172 + 194.d*E (JD2425100 - 29300)
FY    Cyg |[00332]. 130d <= P< = 189d (JD2432500 - 38000).
GG    Cyg |d = 0.079P; Min II 12.1.
GM    Cyg |P var. Min = 2428754.305 + 4.745772d*E (JD2413200 -
GM    Cyg |33500) [01209]; since JD2433500 - see Table.
GN    Cyg |P var. Max = 2425448 + 156d*E (JD2425400 - 27400)
GN    Cyg |[01155]; since JD2427500 - see Table.
GO    Cyg |Min II 8.73. P var. Intrinsic light variability of the
GO    Cyg |components is possible [01210].
GS    Cyg |P = 195d?
GT    Cyg |Depth of Min II 0.05m? P var?
GY    Cyg |Secondary oscillation with P = 4000d and
GY    Cyg |A(V) = 0.5m is possible.
GZ    Cyg |Red.
HL    Cyg |d = 0.02P.
HV    Cyg |VB (Northern component).
HY    Cyg |P var. Max = 2425334 + 344d*E (JD2425300 - 29200)
HY    Cyg |[00332]; since JD2432760 - LB?
II    Cyg |P var. Max = 2425150 + 82d*E (JD2425120 - 25550),
II    Cyg |Max = 2425475 + 94d*E (JD2425550 - 29250) [00332];
II    Cyg |since JD2432500 77d <= P <= 99d.
IK    Cyg |P var. Max = 2425199 + 77.3d*E (JD2425000 - 29200)
IK    Cyg |[00332]; since JD2432500 - see Table.
IT    Cyg |P var. Max = 2425305 + 67.4d*E (JD2425300 - 850)
IT    Cyg |[00332]; since JD2432500 - see Table.
IU    Cyg |B - V: +0.90, +1.45. P var. Max = 2429157.6 + 31.22266d*E
IU    Cyg |(JD2417800 - 29250); Max = 2433601.3 + 31.1550d*E
IU    Cyg |(JD2432700 - 35400); since JD2435400 - see Table.
IV    Cyg |P var. Max = 2425470.406 + 0.33432871d*E (JD2425300 -
IV    Cyg |33120) [03506]; Max = 2434122.519 + 0.33433895d*E
IV    Cyg |(JD2432700 - 40200) [04248]; since JD2440200 - see Table.
IV    Cyg |Shape of the light
IV    Cyg |curve varies: 0.10P <= M - m <= 0.20P.
IX    Cyg |P var. Max = 2425173 + 172d*E (JD2425000 - 25900)
IX    Cyg |[00332]; since JD2428000 - see Table.
KL    Cyg |P var. Max = 2437906 + 536.8d*E (JD2418500 - 38000)
KL    Cyg |[00001]; since JD2438000 - see Table.
KP    Cyg |Delta(S) = 0.
KR    Cyg |Min II 9.37.
KU    Cyg |Min II 11.15; d = 0.047P. Shape of the light curve varies.
KV    Cyg |Min II 11.9.
KY    Cyg |H2O, OH maser.
LN    Cyg |Min II 14.3.
LO    Cyg |Min II 13.3.
LX    Cyg |P var. Max = 2432775 + 460.0d*E (JD2415000 - 33300)
LX    Cyg |[01159]; since JD2437900 - see Table. SC 7/9-e - SC 8/8.5e.
MQ    Cyg |VB A (B 17.5m B, 4.5", 122deg). P var. Max = 2432737 +
MQ    Cyg |428.5d*E (JD2414300 - 33300) [01229]; since
MQ    Cyg |JD2440000 - see Table.
MR    Cyg |Min II 9.12; d = 0.030P; DII = 0.19P.
MU    Cyg |Min II 14.4.
MY    Cyg |Min II 8.99. Min II - Min I = 0.5021P.
MZ    Cyg |P var. Max = 2427641.914 + 21.162460d*E +
MZ    Cyg |0.10575d*10**(-3)*E**2 (JD2414900 - 37900) [03689]; since
MZ    Cyg |JD2443600 - see Table. Probably it is an RV Tau type
MZ    Cyg |variable, and then the period should be doubled [08862].
MZ    Cyg |[A/H] = 0.1.
NQ    Cyg |EW type is possible. Close to V736 Cyg.
NU    Cyg |Min II 14.9.
NZ    Cyg |Min II 14.2.
OS    Cyg |P var.
OU    Cyg |Min II 15.6.
OY    Cyg |Star 23 - 30 [01321].
PP    Cyg |Star G in the chart for VV245 [07749].
PR    Cyg |Star 24 - 40 [01321].
PT    Cyg |Star 23 - 55 [01321].
PU    Cyg |Star 25 - 56 [01321].
PX    Cyg |Star 35 - 78 [01321].
PY    Cyg |Min II 15.2.
QS    Cyg |Min II 13.3.
QT    Cyg |Depth of Min II 0.04m.
QU    Cyg |Min II 15.1.
QW    Cyg |Min II 14.1.
QX    Cyg |Min II 14.5.
V0339 Cyg |np component of a close binary.
V0340 Cyg |Min II 14.5.
V0343 Cyg |[A/H] = -0.2.
V0346 Cyg |Companion 13.8m, 0.4' sf. Min II 11.9. P var.
V0346 Cyg |Min I = 2427270.241 + 2.743345d*E (JD2415000 - 32000);
V0346 Cyg |since JD2432000 - see Table.
V0348 Cyg |According to [07516] EW type variable with large
V0348 Cyg |irregularities: Min = 2441567.177 + 0.285768d*E
V0348 Cyg |(JD2441567 - 95).
V0355 Cyg |Min II 14.3.
V0360 Cyg |P var [06107]. Min I = 2429187.4 + 70.449d*E
V0360 Cyg |(JD2414600 - 34000) [00580]; since JD2426000 - see Table.
V0366 Cyg |Min II 10.2.
V0367 Cyg |VB A (A 0.1", 50deg; B 13.7m, 2.3", 255deg). Min II 7.16.
V0367 Cyg |Shape of the light curve and the radial velocity curve
V0367 Cyg |vary.
V0368 Cyg |According to [00204] EB type (12.8m - 13.8m pg)
V0368 Cyg |with the elements: Min I = 2425808.10 + 0.47586d*E
V0368 Cyg |(JD2425805 - 853).
V0369 Cyg |P var. Max = 2438199 + 104.46d*E (JD2426000 - 38200);
V0369 Cyg |since JD2438200 - see Table.
V0370 Cyg |Min II 11.9. P var. Min I = 2425096.429 + 0.77453979d*E
V0370 Cyg |(JD2414400 - 30000); since JD2430000 - see Table.
V0371 Cyg |Min II 12.5.
V0374 Cyg |d = 0.03P.
V0380 Cyg |Min II 5.76; Min II - Min I = 0.418P (1963).
V0380 Cyg |There are periodic terms in the elements:
V0380 Cyg |+0.8916d*sin(38.8deg + 0.0082deg*E) -
V0380 Cyg |0.0796d*sin(77.6deg + 0.0164deg*E) + 0.0088d*cos(26.4deg +
V0380 Cyg |0.0246deg*E); Min II = 2441262.266 + 12.425612d*E -
V0380 Cyg |0.8916d*sin(38.8deg + 0.0082deg*E) - 0.0796d*sin(77.6deg +
V0380 Cyg |0.164deg*E) - 0.0088d cos (26.4deg + 0.0246deg*E).
V0380 Cyg |Apsidal motion is possible with P = 1490 years.
V0382 Cyg |VB A (B 11.5m, 11", 332deg). Min II 9.12.
V0382 Cyg |Shape of the light curve and depth of Min II vary. P var.
V0382 Cyg |Min I = 2427992.458 + 1.885497d*E (JD2413480 - 29500)
V0382 Cyg |[01253]; since JD2428000 - see Table.
V0385 Cyg |Min II 12.4.
V0387 Cyg |Min II 11.6.
V0388 Cyg |Min II 9.15; d = 0.06P. P var. Min I = 2433584.540 +
V0388 Cyg |0.8590507d*E (JD2427600 - 37200);
V0388 Cyg |since JD2437200 - see Table.
V0389 Cyg |VB A (B 8.0m, 3.4", 305deg, 1980). SB (P = 3.313168d);
V0389 Cyg |Turns around the invisible third companion with
V0389 Cyg |P = 154.09d. According to [01256] the light varies with
V0389 Cyg |two alternate periods P1 and P2. The first oscillation
V0389 Cyg |(P1) with A = 0.19m satisfies the elements: Max =
V0389 Cyg |2423298.460 + 1.12912d*E, the second (P2) with A =
V0389 Cyg |0.05m - the elements: Max = 2429162.080 + 1.19328d*E.
V0389 Cyg |each of them continues for 1 - 3 weeks. At the transition
V0389 Cyg |from one oscillation to the other irregular light
V0389 Cyg |variations are sometimes observed or almost constant
V0389 Cyg |brightness. At the renewal of each oscillation its phase
V0389 Cyg |remains unchanged, experiencing no shift. According
V0389 Cyg |to [08909] in 1975 - 1977 periodicity was not observed.
V0393 Cyg |d = 0.02P.
V0401 Cyg |Min II 11.13. P var. Min I = 2432881.277 + 0.582717d*E
V0401 Cyg |(JD2428800 - 34000); since JD2434000 - see Table.
V0402 Cyg |VB A (B 20", 90deg).
V0407 Cyg |VB A (B 14.0m, 8", 190deg).
V0407 Cyg |Light variations of the Mira type
V0407 Cyg |variable are superimposed by the outburst of the probable
V0407 Cyg |nova which occured near JD2428400 (1936)
V0407 Cyg |with the consequent slow light decrease. Combined spectrum.
V0411 Cyg |P var. Max = 2421075 + 321d*E (JD2421000 - 31100)
V0411 Cyg |[01262]; since JD2431100 - see Table.
V0416 Cyg |Red.
V0425 Cyg |Description of the spectrum and its variations [02685,03149].
V0427 Cyg |P var. Max = 2425471 + 143d*E (JD2425400 - 5950)
V0427 Cyg |[01155]; since JD2433850 - see Table.
V0429 Cyg |In the region of the open cluster NGC 6883.
V0430 Cyg |In the region of the open cluster NGC 6883.
V0430 Cyg |Max = 2425544 + 258d*E (JD2425500 - 27400) [01155].
V0432 Cyg |In the region of the open cluster Dolidze 3.
V0439 Cyg |In the region of the open cluster Berkeley 87 = OCL 161.
V0441 Cyg |Epoch of Min I is given.
V0442 Cyg |Min II 10.4:, d = 0.01P:. According to
V0442 Cyg |[08721] the period given in [00525] must be doubled.
V0443 Cyg |There is a periodic term in the elements:
V0443 Cyg |-0.016d*sin(0.00105*E).
V0444 Cyg |In the H II region S 109. Min II 8.06;
V0444 Cyg |D II  = 0.10P. P var. Min I  = 2430856.453 + 4.21238d*E
V0444 Cyg |(JD2415000 - 30000) [00007]; since JD2430000 - see Table.
V0445 Cyg |P var. Min = 2425527.391 + 1.947833d*E (JD2425500 -
V0445 Cyg |34700) [01155]; since JD2434700 - see Table.
V0447 Cyg |In the region of the open cluster NGC 6871.
V0448 Cyg |In the region of the open cluster NGC 6871. Min II 8.40.
V0450 Cyg |The light curve resembles that of DQ Her.
V0453 Cyg |In the region of the open cluster NGC 6871. Min II 8.68;
V0453 Cyg |d = 0.03P; Min II - Min I = 0.5077P. [07518]. According to
V0453 Cyg |[07518] there is apsidal motion with P = 71 years.
V0454 Cyg |Min II 12.3. In the region of the open cluster IC 4996.
V0455 Cyg |Min II 10.9. P var. Min I = 2431151.908 + 8.7689331d*E
V0455 Cyg |(JD2426800 - 33950) [01286]; since JD2436800 - see Table.
V0456 Cyg |Min II 11.4; Min II - Min I = 0.518P. P var?
V0457 Cyg |Min II 13.9.
V0458 Cyg |Min II 14.2.
V0461 Cyg |PB ~7000d? [08251].
V0462 Cyg |P var. Max = 2428540 + 376.0d*E (JD2416000 - 35200);
V0462 Cyg |since JD2435200 - see Table.
V0463 Cyg |Min II 10.65; Min II - Min I = 0.514P.
V0465 Cyg |There is a close companion of 17.5m.
V0466 Cyg |Min II 11.4.
V0469 Cyg |Min II 12.9; Min II - Min I = 0.57P.
V0470 Cyg |Min II 8.545.
V0471 Cyg |S 5.5/5.5.
V0473 Cyg |P var. Max = 2430615 + 218.5d*E (JD2418000 - 31000)
V0473 Cyg |[00346]; since JD2442300 - see Table.
V0474 Cyg |d = 0.014P.
V0477 Cyg |Min II 8.69; D II = 0.09P; d = 0.003P. P var. Min I =
V0477 Cyg |2429194.309 + 2.3470011d*E (JD2410000 - 29200)
V0477 Cyg |[00001]; Min I = 2437317.2695 + 2.3469943d*E
V0477 Cyg |(JD2429200 - 39700) [08919]; since JD2439700 - see Table.
V0477 Cyg |Apsidal motion with Pi = 349 years; E = 0.302 [06175].
V0477 Cyg |0.331P (1965 - 1970) <= Min II - Min I < = 0.460P (1904).
V0478 Cyg |VB A (B 12.8m, 4", 259deg. Min II 9.02; Min II - Min I =
V0478 Cyg |0.5072P.
V0482 Cyg |VB A (B 14.4m V, M4 III, 8", 225deg).
V0483 Cyg |Min II 11.9.
V0484 Cyg |Min II 13.6.
V0486 Cyg |Min II 14.3.
V0488 Cyg |Min II 13.0.
V0490 Cyg |Min II 13.5; Min II - Min I = 0.47P.
V0491 Cyg |Min II 14.7.
V0493 Cyg |Min II 12.9.
V0494 Cyg |Min II 13.6.
V0496 Cyg |Min II 12.5.
V0498 Cyg |Min II 10.27.
V0500 Cyg |VB B (A 11.5m; 18", 45deg). Min II 12.0.
V0501 Cyg |Min II 13.1; d = 0.02P.
V0502 Cyg |Min II 14.2.
V0505 Cyg |Min II 12.0.
V0509 Cyg |d = 0.05P.
V0512 Cyg |Min II 11.5. There is a periodic term in the elements:
V0512 Cyg |+0.065d*sin(0.2105263deg*(E + 538)).
V0513 Cyg |Min II 12.6.
V0519 Cyg |Min II 13.4.
V0520 Cyg |VB A (B 15", 135deg).
V0525 Cyg |d = 0.03P:.
V0526 Cyg |Min II 13.1. In the region of the open cluster TGC 7039.
V0532 Cyg |P var. Max = 2434618.158 + 3.283651d*E (JD2427900 -
V0532 Cyg |35000); Max = 2436817.694 + 3.282792d*E (JD2435000 -
V0532 Cyg |38700); since JD2438700 - see Table.
V0536 Cyg |d = 0.010P.
V0538 Cyg |B - V: +1.17, +1.50.
V0539 Cyg |P2 = 1500d.
V0541 Cyg |Min II 10.9; DII = 0.012P; Min II - Min I = 0.453P.
V0544 Cyg |P var?
V0546 Cyg |Min II 15.2:; Min II - Min I = 0.48P; d = 0.077P.
V0546 Cyg |In the dark nebula Barnard 144.
V0547 Cyg |B - V: +1.27, +1.73. In the dark nebula Barnard 144.
V0548 Cyg |Min II 8.62. P var. Min I = 2442279.3838 + 1.80524695d*E
V0548 Cyg |(JD2430800 - 42300) [08930]; since JD2442300 - see Table.
V0563 Cyg |P var. Max = 2427590 + 295.4d*E (JD2426000 - 30250);
V0563 Cyg |since JD2430250 - see Table.
V0567 Cyg |d = 0.036P.
V0581 Cyg |Red.
V0586 Cyg |In the region of the open cluster NGC 7039.
V0588 Cyg |VB A (B 18m, 15", 0deg). Very Red.
V0589 Cyg |VB.
V0606 Cyg |P var. Max = 2428376.7 + 50.245d*E (JD2427950 - 31330)
V0606 Cyg |[01262]; since JD2437100 - see Table.
V0612 Cyg |Cycles of 50 - 100d (JD2427950 - 31330) [01262];
V0612 Cyg |since JD2437100 - see Table.
V0614 Cyg |Min II 14.5.
V0618 Cyg |In the region of the open cluster TGC 7092.
V0622 Cyg |In the region of the open cluster NGC 7092.
V0628 Cyg |Min II 12.5.
V0635 Cyg |Min II 13.5.
V0643 Cyg |P var. Elements given in the
V0643 Cyg |Table are valid in the interval JD2427950 - 31330.
V0644 Cyg |VB A (B 15.6m, 6", 141deg; C 16.3m, 6", 141deg).
V0645 Cyg |Observed as the
V0645 Cyg |bright nebular condensation with ~2" diameter scattering
V0645 Cyg |light of an O8 star associated with it but invisible
V0645 Cyg |because of absorption. A part of strongly polarized
V0645 Cyg |bipolar nebula with diameter about 10". There are
V0645 Cyg |strong emission lines of H, Fe II, [O I], [S II], etc. In
V0645 Cyg |the spectrum [08942,09129]. H2O maser source. Infrared
V0645 Cyg |source CRL 2789.
V0651 Cyg |Min II 14.7.
V0652 Cyg |Min II 12.1.
V0664 Cyg |d = 0.05P.
V0666 Cyg |P var. Max = 2427965 + 236d*E (JD2427950 - 31350)
V0666 Cyg |[01262]; since JD2433400 - see Table.
V0670 Cyg |sp component of a close binary.
V0680 Cyg |Min II 10.3.
V0685 Cyg |VB.
V0687 Cyg |Min II 10.4. P var?
V0688 Cyg |d = 0.029P.
V0690 Cyg |d = 0.021P.
V0691 Cyg |d <= 0.034P.
V0692 Cyg |Min II 14.9?
V0693 Cyg |Min II 14.4?
V0694 Cyg |d = 0.017P.
V0695 Cyg |31 Cyg. Probably enters a common system with V1488 Cyg
V0695 Cyg |(32 Cyg). VB A (B 13.0m, 36.8", 332deg; C 6.99m, 107.0",
V0695 Cyg |174deg; D 5.0m, 338", 323deg). d = 0.0151P.
V0695 Cyg |Interferometric binary eclipsing system (A = 0.08",
V0695 Cyg |E = 0.15 [01582]; 0.035", 141.8deg, 1980.4). The epoch of
V0695 Cyg |eclipse of the component of the spectral type B4 by the
V0695 Cyg |component of the type K4 is given in the Table. The
V0695 Cyg |amplitude strongly varies depending upon the wavelength:
V0695 Cyg |A(lambda 6560 A) = 0.03m, A(lambda 3530 A) = 1.80m [09131].
V0696 Cyg |Mean magnitude varies with P = 1600d.
V0700 Cyg |Min II 12.3. P var. Min I = 2432028.863 + 0.340047d*E
V0700 Cyg |(JD2431700 - 37500) [05352]; since JD2437500 - see Table.
V0704 Cyg |Min II 14.2.
V0706 Cyg |Min II 13.9.
V0713 Cyg |Min II 15.1.
V0720 Cyg |P var. Min I = 2427611 + 332d*E (JD2429450 - 32000)
V0720 Cyg |[00798]; since JD2432500 - see Table.
V0726 Cyg |Min II 12.8; d = 0.018P.
V0728 Cyg |P var. Min = 2425760.475 + 2.0601256d*E (JD2425500 - 35000)
V0728 Cyg |[00164]; since JD2439700 - see Table.
V0729 Cyg |VB A (B 13.5m, 1.5", 65deg). Min II 9.29. P var. Min I =
V0729 Cyg |2434264.638 + 6.597700d*E (JD2428700 - 37900)
V0729 Cyg |[00001]; since JD2439750 - see Table.
V0731 Cyg |VB.
V0735 Cyg |Depth of Min II 0.04m.
V0736 Cyg |Min II 16.5. Close to NQ Cyg.
V0737 Cyg |Star 23 - 50 [01321].
V0739 Cyg |Star 36 - 81 [01321].
V0741 Cyg |d = 0.03P.
V0742 Cyg |P var. Max = 2429409.448 + 0.93979d*E (JD2428420 -
V0742 Cyg |30700) [08977]; Max = 2431489.580 + 0.94010d*E
V0742 Cyg |(JD2430250 - 32350); Max = 2433282.014 + 0.93979d*E
V0742 Cyg |(JD2432350 - 33650); since JD2433650 - see Table.
V0742 Cyg |According to [08977] since JD2430700 the observations are
V0742 Cyg |better represented by the elements:
V0742 Cyg |Max = 2432943.701 + 0.93977897d*E - 1.067d*10**(-7)*E**2.
V0747 Cyg |The intervals between maxima of brightness
V0747 Cyg |are 2000 - 4000d. Not red.
V0751 Cyg |In the region of the nebula IC 5070. SB (P = 0.25d [09132]).
V0751 Cyg |Rapid small variations near maximum of brightness
V0751 Cyg |(<B - V> = +0.25) are superimposed sometimes by deep
V0751 Cyg |minima lasting for some hundreds days [02699]. Soft X-ray
V0751 Cyg |source [09133]. Spectrum description [02698,09132].
V0752 Cyg |<B - V> = +0.77, <U - B> = -0.47.
V0753 Cyg |d = 0.12P. P = 0.952374d?
V0757 Cyg |Red.
V0758 Cyg |P = 400d?
V0759 Cyg |P var. Max = 2434513.427 + 0.36001476d*E
V0759 Cyg |(JD2414430 - 34570) [03506]; since JD2434500 - see Table.
V0759 Cyg |Blazhko effect.
V0779 Cyg |Type RR?
V0781 Cyg |P var?
V0783 Cyg |P var. Max = 2433261.029 + 0.62069487d*E
V0783 Cyg |(JD2424690 - 34000); since JD2438970 - see Table.
V0786 Cyg |Usually in minimum brightness, with rapid
V0786 Cyg |brightenings by 0.5m - 1.0m. In the interval JD2427692 -
V0786 Cyg |697 the brightness was 13.5m.
V0789 Cyg |P var? [Fe/H] = -0.91.
V0795 Cyg |sf component of a close pair.
V0796 Cyg |Min II 11.4.
V0797 Cyg |Min 15.4.
V0799 Cyg |P var.
V0801 Cyg |There is a square term in the elements:
V0801 Cyg |+1.93d*10**(-10)*E**2.
V0802 Cyg |P var. Max = 2432779.9342 + 0.59560377d*E
V0802 Cyg |(JD2425480 - 35170) [02775]; Max = 2439415.263 +
V0802 Cyg |0.5955638d*E (JD2435950 - 40000) [09266]. Max =
V0802 Cyg |2440036.409 + 0.595447d*E (JD2440000 - 41000); Max =
V0802 Cyg |2441517.498 + 0.595635d*E (JD2441000 - 42500);
V0802 Cyg |since JD2442500 - see Table. Shape of the light curve
V0802 Cyg |varies (0.13P <=  M - m <= 0.50P); period variations are
V0802 Cyg |accompanied sometimes by strong variations of amplitude
V0802 Cyg |(in the interval JD2440000 - 41000; 0.3m <= A <= 1.7m).
V0803 Cyg |Min II 14.5.
V0806 Cyg |Min II 15.0; DII = 0.061P.
V0807 Cyg |Min II 14.9.
V0808 Cyg |Brightness in maximum varies.
V0809 Cyg |Min II 13.6; DII = 0.069P.
V0810 Cyg |d = 0.050P. Depth of Min II 0.05m. P var?
V0817 Cyg |sp component of the pair.
V0818 Cyg |Shape of the light curve and period vary.
V0821 Cyg |Min II 15.6.
V0822 Cyg |Min II 13.0.
V0824 Cyg |Min II 14.3.
V0825 Cyg |Min II 16.9. Min II = 2433871.915 + 7.709015d*E.
V0826 Cyg |Min II 14.7.
V0828 Cyg |Min II 10.12.
V0832 Cyg |VB A (B 9.43m, 20", 352deg; C 11.62m, 27", 141deg; D 12.72m,
V0832 Cyg |38", 220deg). description of spectral variations [09135].
V0836 Cyg |Min II 8.77. P var. Min I = 2426547.5224 + 0.65341090d*E
V0836 Cyg |(JD2425500 - 42000) [03869]; since JD2441200 - see Table.
V0836 Cyg |Shape of the light curve varies.
V0840 Cyg |LS II 28.3deg [08090]. Cycles 250 - 300d.
V0841 Cyg |Min II 11.2.
V0842 Cyg |Min II 14.1.
V0844 Cyg |VB A (B 17.8m, 2.9", 50deg).
V0850 Cyg |Min II 11.8. P var. Min I = 2430587.263 + 4.5578d*E
V0850 Cyg |(JD2428750 - 30590) [04253]; since JD2434330 - see Table.
V0851 Cyg |d = 0.017P?
V0852 Cyg |Min II 14.9.
V0853 Cyg |Min II 14.2.
V0856 Cyg |Depth of Min II 0.05m.
V0857 Cyg |Depth of Min II 0.03m.
V0859 Cyg |Min II 12.1.
V0865 Cyg |Min II 14.6.
V0866 Cyg |Min II 13.9.
V0869 Cyg |Min II 14.8. Shape of the light curve varies.
V0870 Cyg |Min II 15.8.
V0871 Cyg |Min II 14.9.
V0873 Cyg |Min II 14.7. Min II - Min I = 0.48P.
V0874 Cyg |Min II 13.8.
V0877 Cyg |Min II 12.9.
V0880 Cyg |Min II 14.1; Min II - Min I = 0.506P; d = 0.02P.
V0881 Cyg |Delta(S) is small [09037].
V0882 Cyg |[Fe/H] = -1.42.
V0884 Cyg |np component of a pair. Min II 14.2.
V0885 Cyg |Min II 10.2.
V0886 Cyg |Min II 14.1; Min II - Min I = 0.515P.
V0887 Cyg |Depth of Min II 0.03m.
V0888 Cyg |Min II 15.9.
V0889 Cyg |Min II 10.4.
V0891 Cyg |Min II 9.4.
V0892 Cyg |Min II 15.5. nf component of a close pair.
V0900 Cyg |Min II 15.2.
V0902 Cyg |d = 0.02P. Depth of Min II 0.05m.
V0906 Cyg |Min II 15.7.
V0907 Cyg |Min II 14.9. According to [04427] Min I =
V0907 Cyg |2435066.257 + 0.54138554d*E.
V0908 Cyg |nf component of a close pair. Depth of Min II 0.04m.
V0909 Cyg |Min II 9.66.
V0910 Cyg |Min II 14.2; d = 0.02P.
V0911 Cyg |Min II 14.6. P var? Min I = 2432120.251 + 3.42262215d*E
V0911 Cyg |(JD2415500 - 37900) [04761]; since JD2437100 - see Table.
V0912 Cyg |Depth of Min II 0.05m.
V0913 Cyg |VB A (B 17m, 0deg).
V0920 Cyg |A var. Blazhko effect?
V0922 Cyg |d = 0.02P:.
V0924 Cyg |P var. Max = 2435706.776 + 5.5709816d*E (JD2432760 - 38000)
V0924 Cyg |[08053]; since JD2438000 - see Table.
V0925 Cyg |Min II 16.0.
V0927 Cyg |Epoch of Min brightness is given.
V0928 Cyg |Min II 15.4.
V0931 Cyg |Min II 14.5.
V0932 Cyg |Depth of Min II 0.04m.
V0934 Cyg |Min II 13.7.
V0936 Cyg |Depth of Min II 0.05m.
V0939 Cyg |Min II 12.5.
V0940 Cyg |Min II 15.1.
V0941 Cyg |Min II 13.2.
V0942 Cyg |VB A (B ~10deg, C ~110deg).
V0944 Cyg |np component of pair.
V0947 Cyg |Min II 15.0.
V0948 Cyg |Min II 15.2.
V0949 Cyg |Red.
V0955 Cyg |Min II 15.3. sp component of a close pair.
V0956 Cyg |Min II 15.1. sp component of a close pair.
V0957 Cyg |Min II 12.6.
V0958 Cyg |P = 199d?
V0959 Cyg |Min II 11.4; Min II - Min I = 0.52P; DII = 0.16P:.
V0959 Cyg |sp component of a close pair.
V0961 Cyg |Min II 12.4; Min II - Min I = 0.505P.
V0962 Cyg |d = 0.02P:.
V0964 Cyg |Min II 14.4.
V0965 Cyg |Min II 14.9. Type RRC? P = 0.32028628d?
V0970 Cyg |Min II 14.8.
V0974 Cyg |Min II 12.5; Min II - Min I = 0.462P.
V0974 Cyg |Min II = 2435373.398 + 3.204418d*E.
V0979 Cyg |Min II 14.7.
V0981 Cyg |Min II 15.0.
V0982 Cyg |Red.
V0997 Cyg |[Fe/H] = -0.77.
V1004 Cyg |Min II 13.0.
V1007 Cyg |Depth of Min II 0.04m.
V1008 Cyg |Min II 16.0.
V1010 Cyg |Depth of Min II 0.03m.
V1011 Cyg |Depth of Min II 0.04m.
V1012 Cyg |Min II 15.4.
V1016 Cyg |Before the outburst in 1964 the brightness
V1016 Cyg |changed between 15.0m and 17.5m pg [05701], the spectral
V1016 Cyg |type was late Me alpha [01222]. In the 1964 - 67 the
V1016 Cyg |brightness increased from 16.0m to 11.2m B. In 1967 - 69
V1016 Cyg |the brightness steadily increased to 10.05m B,
V1016 Cyg |being constant in V system (10.5m). In the infrared it
V1016 Cyg |changes in the limits 6.9 - 8.4 J, 4.7 - 5.8 K with the
V1016 Cyg |period 470d [07174,09141]. High excitation emission
V1016 Cyg |spectrum with strong IR excess resembles that of
V1016 Cyg |symbiotic variables [09142]. X-ray and radio source.
V1018 Cyg |Min II 11.6.
V1021 Cyg |Min II 14.3.
V1023 Cyg |Min II 12.9; d = 0.03P:. DII = 0.14P.
V1023 Cyg |Min II - Min I = 0.495P.
V1024 Cyg |Depth of Min II 0.04m.
V1030 Cyg |Elements given in the
V1030 Cyg |Table are valid in the interval JD2426600 - 32300.
V1033 Cyg |P var.
V1034 Cyg |Min II 9.9.
V1035 Cyg |P var?
V1037 Cyg |Min II 14.8.
V1038 Cyg |VB B (9.4", 215deg, 1963). Min II 15.5.
V1039 Cyg |Min II 15.6.
V1042 Cyg |VB A (B 10m, 53", 110deg). In HII region S 109.
V1044 Cyg |Min II 16.5.
V1045 Cyg |Min II 16.0.
V1047 Cyg |d = 0.02P.
V1053 Cyg |d = 0.05P.
V1057 Cyg |In the dark nebula, in the region of the North America
V1057 Cyg |nebula (NGC 7000). In 1969 - 70 (JD2440400 - 830)
V1057 Cyg |the outburst from 16.5m to 10.3m occured. Brightness
V1057 Cyg |maximum was observed at JD2440830 (spectrum - B3).
V1057 Cyg |Before the outburst the light changed in the range
V1057 Cyg |15.5m - 16.5m, the spectral type was Ke with
V1057 Cyg |characteristic features of T Tau type stars [02698,06415].
V1057 Cyg |After the outburst the brightness began to weaken
V1057 Cyg |monotonouosly and in 1982 reached 13.1m B (the spectral
V1057 Cyg |type about G2 - G5 Ib). Strong Halpha emission appeared
V1057 Cyg |in 1971. There are also small rapid light fluctuations.
V1057 Cyg |Description of light variations [06504,07115,
V1057 Cyg |07754, 08996]. The star is associated with a luminous
V1057 Cyg |arc-shaped reflection nebula. This nebula with length
V1057 Cyg |of about 3' appeared in 1971 and its brightness is
V1057 Cyg |gradually decreasing simultaneously with the fading
V1057 Cyg |of the star.
V1061 Cyg |Min II 9.5.
V1063 Cyg |P var. Max = 2428260 + 339d*E (JD2428260 - 30700);
V1063 Cyg |since JD2433500 - see Table.
V1064 Cyg |Min II 15.3.
V1068 Cyg |Min II 11.2; d = 0.070P.
V1068 Cyg |A migrating wavelike distorsion with an amplitude ~0.1m V
V1068 Cyg |is being observed outside eclipses [08999].
V1073 Cyg |Min II 8.57.
V1074 Cyg |Min II 14.8.
V1083 Cyg |Min II 11.2.
V1085 Cyg |Observations given in [07010] contradict the elements given
V1085 Cyg |in [07193]: Min = 2437856.592 + 2.8089d*E.
V1096 Cyg |d = 0.03P.
V1102 Cyg |Radio-quiet N galaxy. Absorption spectrum without emission
V1102 Cyg |lines; z = 0.0272.
V1111 Cyg |Blazhko effect is possible.
V1122 Cyg |Blazhko effect is possible.
V1130 Cyg |Min II 12.9.
V1136 Cyg |Min II 13.2. Eccentric orbit (E = 0.3). Apsidal motion is
V1136 Cyg |possible [08051].
V1141 Cyg |Min II 11.8.
V1142 Cyg |Min II 13.4.
V1143 Cyg |Min II 6.06; Min II - Min I = 0.743P; d = 0.002P.
V1157 Cyg |Min II 13.6.
V1158 Cyg |d = 0.02P; Depth of Min II 0.04m.
V1161 Cyg |d = 0.01P.
V1162 Cyg |Only one Max was observed (see Table). Thereafter - either
V1162 Cyg |invisible, or fairly constant (17.6m - 17.8m). Bluish.
V1171 Cyg |VB A (B 11.0m, 0.34", 71.2deg; 1979.5). Min II 10.3.
V1175 Cyg |Min II 16.5. P var. Min I = 2434629.545 + 1.3330d*E
V1175 Cyg |(JD2426620 - 34630); since JD2434635 - see Table.
V1176 Cyg |VB. Variable is probably the northern red component.
V1187 Cyg |In the nebula IC 1318B. Min II 11.19. P = 3.7675d?
V1188 Cyg |Min II 14.3.
V1189 Cyg |Min II 13.7. P var. Min I = 2437906.516 + 1.041908d*E
V1189 Cyg |(JD2426620 - 31240); since JD2437906 - see Table.
V1191 Cyg |In the nebula IC 1318B. VB A (B 13m, 11", 299deg; C 13m,
V1191 Cyg |11", 284deg). Min II 11.11. Shape of the light curve varies.
V1193 Cyg |Min II 14.3.
V1196 Cyg |Depth of Min II 0.05m.
V1200 Cyg |Min II 16.1:.
V1210 Cyg |Red.
V1212 Cyg |Red.
V1218 Cyg |VB A (B 17m, sf).
V1225 Cyg |VB A (B 16m V, B - V = +1.3m, 1.2", 270deg; C 15.0m V,
V1225 Cyg |B - V = +0.5m, 2.4", 270deg); P var? Max = 2428250 +
V1225 Cyg |384.2d*E (JD2428200 - 38250) [03160]; since
V1225 Cyg |JD2438500 - see Table.
V1236 Cyg |Red.
V1255 Cyg |Brightness in Max varies in the range 15.2m - 16.0m with
V1255 Cyg |possible elements: Max = 2439382.281 + 0.28619537d*E.
V1256 Cyg |Min II 14.1.
V1273 Cyg |Min II 16.5.
V1275 Cyg |In the region of the open cluster NGC 6819.
V1281 Cyg |Min II 15.4.
V1285 Cyg |Red.
V1302 Cyg |Depth of Min II 0.05m.
V1305 Cyg |Min II 11.5m - 11.7m (var).
V1307 Cyg |Considerable dispersion of mean light curve points.
V1315 Cyg |Min II 15.3.
V1316 Cyg |(P) > 100d.
V1318 Cyg |LkH alpha 225. Associated with a cometary nebula.
V1321 Cyg |P = 0.7281802d?
V1322 Cyg |In the region of the open cluster NGC 6913.
V1326 Cyg |Min II 11.8; Min II - Min I = 0.53P.
V1327 Cyg |Very red.
V1329 Cyg |In 1891 - 1964 light variations in the range 14.2m - 15.5m
V1329 Cyg |with deep minima to 18m; the minima are satisfied by the
V1329 Cyg |elements given in the Table; D = 0.1p; spectral type M
V1329 Cyg |[07235]. In 1964 - the outburst up to 12.1m. Then gradual
V1329 Cyg |brightness decrease superimposed by periodical
V1329 Cyg |variations with an amplitude near 1m. Light minima
V1329 Cyg |as before are satisfied by the elements given in the
V1329 Cyg |Table but the character of eclipses changed (probably
V1329 Cyg |because of appearance of a dense envelope ejected
V1329 Cyg |by one of the components of the system). After the
V1329 Cyg |outburst high excitation emission spectrum with IR
V1329 Cyg |excess is observed similar to the spectrum of symbiotic
V1329 Cyg |variables.
V1331 Cyg |Associated with a cometary nebula.
V1334 Cyg |VB A (B 7.9m, B5 - B8, 0.13", 26.1deg, 1975).
V1336 Cyg |According to [07010], RR? P = 0.5d?
V1341 Cyg |Cyg X-2. SB1. Halo object (nu = -220 km/s). Strong
V1341 Cyg |reflection effect changes the spectral type of the F
V1341 Cyg |component. Spectral line profiles vary. The lines of
V1341 Cyg |He II, KCa II, C III,and N III are in emission. The
V1341 Cyg |system has low and high states. During the low state the
V1341 Cyg |mean light curve is a double wave with the range
V1341 Cyg |15.1m - 15.4m B. Epoch of Min I given in the Table
V1341 Cyg |corresponds to the F star in superior conjunction;
V1341 Cyg |Min II 15.4. The eclipse of the accretion disk at the
V1341 Cyg |phase 0.5P in partial. Rapid light variability by 0.1m
V1341 Cyg |in 10 minutes and by 0.5m in several hours is
V1341 Cyg |superimposed. In the high states lasting
V1341 Cyg |for ~10d the mean light increases by 0.5m. Radio
V1341 Cyg |source at 8085 MHz, source of soft and hard X-ray
V1341 Cyg |emission from 0.1 to 60 KeV.
V1345 Cyg |Min II 15.0:.
V1354 Cyg |Depth of Min II 0.04m.
V1356 Cyg |Min II 10.4.
V1357 Cyg |Cyg X-1. SB1. The epoch of the inferior conjunction of the
V1357 Cyg |optical component is given in the Table. Min II 8.88. The
V1357 Cyg |shape of the light curve varies; Min II sometimes are not
V1357 Cyg |observed. The periodicity in the light curve variations
V1357 Cyg |as well as in polarization changes is possible with
V1357 Cyg |P = 78.4d [09021,09022]. Rapidly variable X-ray source in
V1357 Cyg |wide range up to 3 MeV characterized by the change of high
V1357 Cyg |and low states. Light and X-ray variation with P = 294d
V1357 Cyg |is also detected [09154,09156]. Variable and flare radio
V1357 Cyg |source at 2695 and 8085 MHz.
V1372 Cyg |P2 = 360d?.
V1374 Cyg |Min II 17.7.
V1384 Cyg |In the region of the open cluster NGC 6913.
V1396 Cyg |VB AB (10.26m V, 12.3m V; A = 0.1127", P = 29.33 Y
V1396 Cyg |[09026]); mu = 0.67", P = 113deg; A-SB 2 (mAb - mAa = 0.6m,
V1396 Cyg |P = 3.275631d [09025]). Probably all the three components
V1396 Cyg |of the system are variables of the UV Cet type, and
V1396 Cyg |according to [05716] also of the BY Dra type. The range of
V1396 Cyg |combined brightness of the system is given in the Table.
V1396 Cyg |Really the flare of AB component was observed in the
V1396 Cyg |spectrograms [09025].
V1401 Cyg |Min II 13.6.
V1410 Cyg |P > 400d.
V1411 Cyg |P = 1.553478d?
V1412 Cyg |Min II 15.5.
V1414 Cyg |Northern component of a close pair; d = 0.04P.
V1416 Cyg |Min II 14.7.
V1417 Cyg |Min II 13.1.
V1421 Cyg |In the region of the planetary nebula NGC 6857 = K3 - 50.
V1425 Cyg |Depth of Min II 0.31m.
V1427 Cyg |In the region of the open cluster M39.
V1429 Cyg |Min II 15.3.
V1430 Cyg |Min II 15.0.
V1436 Cyg |Min II 15.9, D II = 0.08P; Min II - Min I = 0.48P.
V1437 Cyg |Min II 16.0.
V1440 Cyg |In the region of the open cluster NGC 6819.
V1465 Cyg |Resembles an eclipsing variable.
V1478 Cyg |VB A (B 17m:, 3", 80deg).
V1478 Cyg |Compact radio source. extended structure centered at the
V1478 Cyg |star is observed at 5 Ghz. Bq [] star with the excess of
V1478 Cyg |infrared radiation of dust at T = 300degK. Description of
V1478 Cyg |the spectrum [07080,07081,07523,09159,09160].
V1479 Cyg |In the region of the nebula IC 5070.
V1481 Cyg |Min II 12.5. In the region of the open cluster NGC 7128.
V1485 Cyg |Identical to VES 28, as it follows from latter star's
V1485 Cyg |coordinates and magnitudes in [7095], but the star is
V1485 Cyg |actually invisible in the chart in [7095], where a faint
V1485 Cyg |companion, to 0.4'N of the variable, is erroneously marked.
V1485 Cyg |Similarly, it is identical to +29deg 104, judging from the
V1485 Cyg |latter star's photometry and spectral type from [4732];
V1485 Cyg |however, the star is plotted slightly offset (by 0.8' to E)
V1485 Cyg |in the chart in [4732].
V1488 Cyg |32 Cyg. Probably enters a common system with V695 Cyg
V1488 Cyg |(31 Cyg). 0 < d < 0.011P. P var.
V1488 Cyg |Min I  = 2420670.0 + 1140.1d*E (JD2411400 - 29700).
V1488 Cyg |Since JD2429700 - see Table.
V1488 Cyg |The epoch of the eclipse of the B4 type
V1488 Cyg |Component by the K5 type component is given. There
V1488 Cyg |is also small physical light variability of the K
V1488 Cyg |component [08896,09161]. Depth of eclipses depends of lambda:
V1488 Cyg |0.04M V, 0.13m B, 0.27m (lambda 4243A),0.90m (lambda 3552A).
V1489 Cyg |NML Cyg. 17.0m: - 18.0m V, B>21M; I - K = +8.17.
V1489 Cyg |Very large IR exess due to expanding gaseous-dust envelope.
V1489 Cyg |In the area 2.5"*3.5" around
V1489 Cyg |the star the system of about 60 discrete sources of
V1489 Cyg |OH emission is detected [07461]; source of OH, H2O,
V1489 Cyg |SiO maser emission. Light variations are periodical
V1489 Cyg |(see also [09163]). The object may be a protostar being
V1489 Cyg |observed at the end of condensation process. The late
V1489 Cyg |spectrum arises probably in the extending envelope
V1489 Cyg |[09165,09166].
V1490 Cyg |In the region of the nebula IC 5070.
V1491 Cyg |In the region of the nebula IC 5070.
V1492 Cyg |In the region of the nebula IC 5070.
V1493 Cyg |In the region of the nebula IC 5070. V1707 Cyg 10.5"P.
V1494 Cyg |In the region of the nebula IC 5070.
V1495 Cyg |In the region of the nebula NGC 7000.
V1497 Cyg |In the region of the nebula NGC 7000.
V1498 Cyg |In the region of the nebula NGC 7000.
V1500 Cyg |In August 1975, before the very rapid increase
V1500 Cyg |of light, the brightness of the Nova gradually increased
V1500 Cyg |from 17.6m to 13.5m B (JD2442632 - 653.2). After Max
V1500 Cyg |almost monotonous decay of brightness is superimposed by
V1500 Cyg |light variations with the amplitude of 0.03m - 1.0m V;
V1500 Cyg |the period of these variations in the interval
V1500 Cyg |JD2442656 - 43100 changed in the range 0.1415d [09167,
V1500 Cyg |09168] - 0.137d [09169,09170].  Since JD2443100 Min =
V1500 Cyg |2443696.4827 + 0.1396133d*E. Some investigators (see,
V1500 Cyg |for instance, [09173]) adopt double value of this peiod.
V1500 Cyg |A month after the light maximum of the Nova the
V1500 Cyg |radio emission was registered at 2695 and 8085 MHz [09171].
V1507 Cyg |The epoch of a broad Min I (superior conjunction of
V1507 Cyg |the B component) is given; Min II 7.01; D II = 0.20P,
V1507 Cyg |Min II - Min I  = 0.29P; e = 0.39. Unusual light curve
V1507 Cyg |[08213,09049]. Shape of the light curve and depths of
V1507 Cyg |Min vary. Gaseous streams And expAnding envelope.
V1508 Cyg |Min II 13.3.
V1509 Cyg |VB A (B 11.7m, 55", 106deg).
V1511 Cyg |V - K = 13.6m.
V1513 Cyg |Gliese 781; mu alpha = -0.146S, mu delta = -1.00"; SB.
V1515 Cyg |In a dark nebula,  near the nebula NGC 6914. Connected
V1515 Cyg |with nebular appendage like a Comma. Light increase was
V1515 Cyg |observed from 1944 till 1958. Since 1958 the star is in
V1515 Cyg |Max. Slow light variations with A <= 1.6m. The absorption
V1515 Cyg |line Li I lambda 6707A is seen in the spectrum.
V1521 Cyg |Cyg X-3. Peculiar infrared X-ray source. V > 23m.
V1521 Cyg |Flare radio source. In the K band short and slow flares
V1521 Cyg |on the time scale about 2 minutes and 1-2 hours,
V1521 Cyg |irregular variations and longperiodic variability are
V1521 Cyg |observed [07752]. These variations are accompanied
V1521 Cyg |by periodical oscillations of infrared, X-ray and gamma
V1521 Cyg |radiation with the elements: Min = 2440949.8986 +
V1521 Cyg |0.1996830d*E + 1.25d*10**(-10)*E**2 [09187]. Usually the
V1521 Cyg |amplitude of these variations A(K) = 0.5m, but sometimes
V1521 Cyg |they disappear completely.
V1523 Cyg |Amplitude and mean brightness strongly vary.
V1531 Cyg |LkH alpha 142. VB A (B = V1532 Cyg, 2.5", 90deg). In the
V1531 Cyg |region of the nebula IC 5070. Combined brightness and
V1531 Cyg |spectrum are given.
V1532 Cyg |LkH alpha 143. VB B (A = V1531 Cyg; B 2.5", 90deg).
V1532 Cyg |In the region of the nebula IC 5070. Combined brightness
V1532 Cyg |and spectrum are given.
V1535 Cyg |In the region of the nebula IC 5070.
V1536 Cyg |In the region of the nebula NGC 7000.
V1538 Cyg |In the region of the nebula NGC 7000.
V1539 Cyg |In the region of the nebula NGC 7000.
V1540 Cyg |In the region of the nebula NGC 7000.
V1546 Cyg |In the region of the nebula NGC 7000.
V1548 Cyg |VB A (B 16.7m, 6.2", 131deg).
V1554 Cyg |VB A (B 14.7m, 3.5", 214deg).
V1577 Cyg |In the cluster and nebula IC 5146.
V1578 Cyg |In the cluster and nebula IC 5146. VB A (B 15m, 5", 45deg;
V1578 Cyg |C 17m, 5", 225deg). Associated with a reflecting nebula.
V1580 Cyg |There is a periodic term in the elements:
V1580 Cyg |-0.027d*sin(0.045deg) (JD - 2439000).
V1581 Cyg |G 208 - 44. VB A (B = G 208 - 45, 15.97m V, M6Ve; 7.9",
V1581 Cyg |106deg, 1954; 8.2", 96deg, 1974). mu = 0.71", P = 140deg.
V1581 Cyg |The flare was observed during spectroscopic observations
V1581 Cyg |[09175]. The companion may be also a UV Cet type variable.
V1581 Cyg |The range of combined brightness variation of the system
V1581 Cyg |is given.
V1584 Cyg |Epoch of min brightness is given.
V1597 Cyg |In the region of the nebula IC 5070.
V1598 Cyg |In the region of the nebula IC 5070.
V1600 Cyg |In the region of the nebula IC 5070.
V1608 Cyg |In the region of the nebula NGC 7000.
V1610 Cyg |Infrared source CRL 2688, the star of the spectral type
V1610 Cyg |F5Ia, associated with a bipolar reflection nebula
V1610 Cyg |(the so-called Egg nebula). The northern component of
V1610 Cyg |the nebula is 4" to the north from the source. Since 1920
V1610 Cyg |to 1958 the integrated light of this component increased
V1610 Cyg |from 15.2m to 13.4b B and after that does not vary [08735]. Light
V1610 Cyg |of the faint (16.2m B) southern component (5" to the
V1610 Cyg |south from the source) varies by 0.6m B [09176]. The
V1610 Cyg |radiation of the nebula is strongly polarized (46%,
V1610 Cyg |theta = 106deg in V system). There are C3 absorption
V1610 Cyg |features as well as Na, C2, and [S II] emission in the
V1610 Cyg |spectrum. Probably the object is a precursor of a
V1610 Cyg |planetary nebula [09178].
V1611 Cyg |In the region of the nebula NGC 7000.
V1624 Cyg |A var.
V1624 Cyg |In 1957 out of a B star turned into Be star. Probably must
V1624 Cyg |be referred also to GCAS type.
V1661 Cyg |VB A (B 11.14m, 20", 174deg).
V1668 Cyg |There are sinusoidal light variations with A(V) = 0.15m
V1668 Cyg |and elements Min = 2443767.475 + 0.4392d*E in the
V1668 Cyg |descending branch of the light curve after JD2443765
V1668 Cyg |[09179]. Infrared light curves (1.6 - 10 mkm) have a
V1668 Cyg |secondary maximum (JD2443815) due to the formation of
V1668 Cyg |the dust envelope. At 10 mkm this secondary maximum is
V1668 Cyg |brighter than the primary one [09069].
V1669 Cyg |d = 0.036P.
V1671 Cyg |Delta(U) = 0.06.
V1674 Cyg |VB (B 15m, 5").
V1674 Cyg |The range of combined brightness variation is given. It
V1674 Cyg |is not excluded that it is the component B that is
V1674 Cyg |variable. Slow variations of mean brightness in the range
V1674 Cyg |10.555m - 10.570m B are superimposed by sinusoidal
V1674 Cyg |periodikal ones with P1 = 1.3608d (A1 = 0.0037m)
V1674 Cyg |and P2 = 0.8055d (A2 = 0.0032m).
V1676 Cyg |In the open cluster NGC 6871.
V1676 Cyg |ADS 13374 A (B 12.0m, 6.5", 64deg; C 11.0m, 9.5", 28deg
V1676 Cyg |D 9.5m, B3V, 11.4", 301deg; E 11.42m, 28.1", 109deg;
V1676 Cyg |F 7.36m, B1IA, 35.9", 29deg); SB2 (P = 112.7d).
V1696 Cyg |SB1 (Porb = 4.3174d). Epoch of Min brightness is given.
V1696 Cyg |The eclipse of the accretion disc around the compact
V1696 Cyg |object formed in the outburst of a Supernova in a binary
V1696 Cyg |system about 5*10**6 years ago is possible [03619].
V1701 Cyg |In the region of the nebula IC 5070.
V1702 Cyg |In the region of the nebula IC 5070.
V1703 Cyg |In the region of the nebula IC 5070.
V1704 Cyg |In the region of the nebula IC 5070.
V1706 Cyg |In the region of the nebula IC 5070.
V1707 Cyg |In the region of the nebula IC 5070. V1493 Cyg 10.5"f.
V1711 Cyg |In the region of the nebula NGC 7000.
V1716 Cyg |In the region of the nebula NGC 7000.
V1719 Cyg |Shape of the light curve varies.
V1720 Cyg |Min II 7.79.
V1721 Cyg |P var.Min I = 2442605.497 + 2.724370d*E (JD2442311 - 928);
V1721 Cyg |since JD2442928 - see Table.
V1722 Cyg |Min II 14.6?
V1726 Cyg |Possible member of an anonimous open cluster.
V1727 Cyg |4U 2129 +47. Lx/Lopt ~10.
V1727 Cyg |Emissions in the spectrum: NeII lambda 4686A, CIII - NIII
V1727 Cyg |lambda lambda 4640 - 50A.
V1735 Cyg |In the complex of dark nebulae associated with the
V1735 Cyg |open cluster and the nebula IC 5146. Lights up a
V1735 Cyg |reflecting nebula. Became brighter by 5m at least
V1735 Cyg |from 1952 to 1965.
V1737 Cyg |B - V = +3.7.
V1738 Cyg |B - V = +5.5:.
V1739 Cyg |B - V = +4.5:.
V1744 Cyg |Epoch of Max in U system is given.
V1746 Cyg |Sometimes P = 0.21d is observed.
V1747 Cyg |P > 100d. B - V = +4.0.
V1748 Cyg |In the nebula IC 1318a.
V1751 Cyg |In the nebula IC 1318c.
V1761 Cyg |Close companion? Elements are not certain.
V2105 Cyg |Variability type and spectral type (F8Iab:) do not agree.
V2121 Cyg |Strong Blazhko effect.
V2150 Cyg |Type RR: is also possible.
V2174 Cyg |SB, Porb = 225.162d.
V2175 Cyg |X-ray source.
V2312 Cyg |Erroneously called HD 192776 in [190].
V2324 Cyg |Possible brightening trend over 6 years, maybe due to dissipating
V2324 Cyg |dust envelope, plus quicker variations.
alf   Cyg |VB A (B 11.4m, 75.3", 106deg).
tau   Cyg |VB A (B 6.44m, G1V, A = 0.88", P = 49.80yr; C 12.20m,
tau   Cyg |29", 230deg). 0.083d <= P <= 0.125d.
tau   Cyg |The range of total light variation is given.
ups   Cyg |VB A (B 10.2m, 15.2", 220deg; C 10.2m, 21.5", 180deg).
khi   Cyg |VB A (B 10.8m, 158", 254deg). S 6 + %1e (Tc). SiO
khi   Cyg |maser. P var.Max = 2393559 + 405.88d*E (JD2337150 - 94000);
khi   Cyg |since JD2394000 - see Table.
P     Cyg |The appearance of the star was firstly noted in
P     Cyg |1600, when its brightness was 3m. Since the XVIII
P     Cyg |century the light of the star varies in the range
P     Cyg |4.6m - 5.6m vis. Radio source at the millimetre and
P     Cyg |centimetre wavelengths.
Q     Cyg |In minimum brightness varies periodically with the
Q     Cyg |amplitude 0.5m: Max = 2440495 + 54.99d*E; P = 64.81d is
Q     Cyg |also possible. Mean level of brightness varies in the
Q     Cyg |range 15.2m - 15.9m B.
S     Del |VB A (B 56", 342deg). Double maxima are sometimes observed.
U     Del |Mean brightness var, P = 1100d. According to [08993], the
U     Del |period value 160d - 180d is more likely than 110d.
W     Del |d = 0.017P. Min II 9.79. P var. Since JD2433000 - see
W     Del |Table. The light curve shape var.
RZ    Del |VB (A var; B var, 17", 137deg) [03771].
TT    Del |P var. Since JD2435000 - see Table.
TW    Del |Delta(m) var (0.5m + 3.4m).
TW    Del |The light curve resembles that of RV Tau, with Min I and
TW    Del |Min II; the epoch of Min I is given.
TW    Del |Min I = 2432171.1 + 118.4d*E (1947 - 1952);
TW    Del |Min I = 2435386.8 + 115.9d*E (1955 - 1963); during
TW    Del |1964 - 1970 - see Table.
TX    Del |P var. P = 6.166585d (JD2428000 - 36600); since
TX    Del |JD2436600 - see Table.
TY    Del |Min II 9.8. P var.Min = 2428020.399 + 1.191121d*E
TY    Del |(JD2428000 - 38000) [00279]; since JD2438000 - see Table.
TZ    Del |Epoch of Min is given.
VV    Del |Depth of Min II 0.05m.
YY    Del |Min II of the depth ~0.05m is possible. P var.
YY    Del |Min = 2425795.488 + 0.7930856d*E (JD2425000 - 34000)
YY    Del |[01329]; since JD2434000 - see Table.
AL    Del |Min II 12.4.
BG    Del |Min II 13.8.
BK    Del |P var?
BR    Del |Emission.
BX    Del |Delta(S) = 0.
BY    Del |Min II 11.8.
CE    Del |[Fe/H] = -0.68.
CF    Del |The light curve shape var?
CH    Del |[Fe/H] = -1.23. According to [09037], P = 0.315D.
CN    Del |Min II 14.6.
CR    Del |Min II 13.7.
CS    Del |[Fe/H] = -0.92.
CU    Del |Abrupt phase chande was noted.
CW    Del |P var.P = 0.58209d (JD ~2427100), P = 0.58211D
CW    Del |(JD ~2428800); During JD2429800 - 30600 - see Table.
DG    Del |The elements should be checked.
DK    Del |Min II 14.2.
DM    Del |Min II 8.80.
DT    Del |Epoch od Min is given. The elements are valid during
DT    Del |JD2425480 - 6260.
DX    Del |[Fe/H] = -0.11.
EG    Del |P var. Max = 2425535.42 + 0.3248545d*E (JD2425478 - 30619)
EG    Del |[00911]; abrupt change near JD2432578, since then see Table.
EI    Del |The mean brightness var, P ~600d.
EK    Del |B - V: +0.29, +0.53.
ES    Del |Epoch of Max from [03715], [07527] contradict the given
ES    Del |elements.
ET    Del |Min II 12.7.
EW    Del |Min II 15.5.
EX    Del |Min II 13.3.
FI    Del |Min II 14.5.
FK    Del |Min II 14.5.
FM    Del |Delta(S) = 0.
FP    Del |[Fe/H] = -1.44.
FR    Del |Min II 15.3.
FT    Del |Blazhko effect?
GG    Del |Min II 12.6. P var?
GN    Del |P var? Delta(m) var?
GY    Del |VB B (A = BD +15deg 4134A, SP A - F).
HR    Del |Porb = 0.170920d. The brightness began to increase on
HR    Del |JD ~2439653. Waves with maxima on JD2439752 (4.55m),
HR    Del |2439799 (4.64m), followed by a sharp main Max, flat max on
HR    Del |JD2439981 (4.09m) and final decline. Radio source.
HU    Del |mu = 0.685", theta = 79deg. Astrometric binary
HU    Del |(semiamplitude of deviations 0.118", Porb = 1.52yr).
II    Del |[Fe/H] = -1.30.
IO    Del |A single outburst  was observed (JD2439378 - 388).
IV    Del |D ~0.1d.
LS    Del |Min II 8.76.
del   Del |(k - b)2 = 0.19. SB2 (Porb = 40.58d; e = 0.7).
del   Del |Spectra of both SB components show Am features; Fe, Ca,
del   Del |Sc deficiency, Sr, Y, Zr, Ba, Ce, La, Eu excess.
del   Del |Both components are DSCT variables; the period of the
del   Del |main component pulsation is 0.158d, that of the
del   Del |secondary is 0.134d [07528]. Any of the oscillations may
del   Del |occasionally dominante in the combined brightness:
del   Del |according to [07529], Max = 2439338.4444 + 0.135547d*E;
del   Del |according to [07530], P = 0.154991d.
R     Dor |VB A (B 11.9m, 34", 10deg; C 11.0m, 35", 130deg, 1933).
R     Dor |H2O, SiO, HC3N emission.
S     Dor |VB A (B 12.1m, 13"). The member of the large magellanic
S     Dor |cloud. In the cluster NGC 1910 and a diffuse nebula.
S     Dor |One of the absolutely brightest stars. Deep Min: 1891,
S     Dor |1900, 1930, 1940, 1955, 1964.
T     Dor |VB A (B 12.0m vis, 5", 13deg.)
V     Dor |At the edge of the Large Magellanic Cloud.
RR    Dor |In the region of the Large Magellanic Cloud. Min II 14.5.
RW    Dor |In the region of the Large Magellanic Cloud.Cloud
RW    Dor |non-member. P var [09036]. Min II 11.2.
RX    Dor |In the region of the Large Magellanic Cloud. Cloud
RX    Dor |non-member?
SW    Dor |In the region of the Large Magellanic Cloud.
SW    Dor |Cloud non-member. P var [09036].
SX    Dor |In the region of the Large Magellanic Cloud,
SX    Dor |Cloud non-member. Delta(m) var.
SY    Dor |In the region of the Large Magellanic Cloud.
SY    Dor |According to [09036], variability is doubtful.
SZ    Dor |In the region of the Large Magellanic Cloud, cloud
SZ    Dor |non-member.
TY    Dor |In the region of the Large Magellanic Cloud, cloud
TY    Dor |non-member.
UU    Dor |In the region of the Large Magellanic Cloud,cloud
UU    Dor |non-member.
UV    Dor |In the region of the Large Magellanic Cloud,cloud
UV    Dor |non-member.
UX    Dor |In the region of the Large Magellanic Cloud, cloud
UX    Dor |non-member.
XX    Dor |In the region of the Large Magellanic Cloud, cloud
XX    Dor |non-member. [Fe/H] ~-1.3.
ZZ    Dor |In the region of the Large Magellanic Cloud, cloud
ZZ    Dor |non-member.
AA    Dor |d = 0.02P. Min II 11.21.
alf   Dor |VB A (B 4.3m, A = 0.2125", P = 13.00yr.)
alf   Dor |The range of combined brightness variations is given.
bet   Dor |P var. Current elements are given.
T     Dra |ADS 10937 A (B = UY Dra, optical, 16", 222deg).
U     Dra |P var. Mean elements are given.
W     Dra |P var. Max = 2416748 + 257.11d*E (JD2416750 - 21390);
W     Dra |Max = 2430826 + 262.11d*E (JD2421390 - 30820);
W     Dra |Max = 2439962 + 268.87d*E (JD2430820 - 40490);
W     Dra |since JD2440490 - see Table.
Y     Dra |According to visual observations, 7.8m - 15.0m.
Z     Dra |Min II 11.0. P var. Min = 2430973.314 + 1.3574176d*E
Z     Dra |(JD2428460 - 33300); Min = 2433268.708 + 1.357440d*E
Z     Dra |(JD2433300 - 43500); since JD2443500 - see Table.
RR    Dra |d = 0.015P. Min II 10.1. P var. Before JD2439000
RR    Dra |Min I = 2433390.458 + 2.83123d*E [01001];
RR    Dra |since JD2440000 - see Table.
RS    Dra |During JD2436012 - 37584 P = 145.3d.
RS    Dra |Delta(m) and the light curve share vary strongly.
RW    Dra |P var. Mean elements are given.
RW    Dra |Composite Blazhko effect;
RW    Dra |Pi = 93.95P = 41.61d; Pi1 = 280P; Pi2 = 6140P; Pi3 =
RW    Dra |3400P [01585]. 0.11P <= M - m <= 0.32P. Delta(S) = 3.
RX    Dra |Min II 10.3, d II = 0.009P.
RZ    Dra |Min II 10.38. P var. Min = 2429448.787 + 0.55087668d*E
RZ    Dra |(1907 - 1968) [03822]; since 1968 - see Table.
SU    Dra |P var. Before 1955 Max hel = 2420605.762 +
SU    Dra |0.66041890D; since 1955 - see Table. [Fe/H] = -1.39.
SW    Dra |Delta(S) = 3.5.
SX    Dra |d = 0.035P. Min II 10.0. P var. Min I = 2432273.276 +
SX    Dra |5.1692d*E (JD2432000 - 38000); since JD2442000 - see Table.
TT    Dra |P2 = 198d.
TW    Dra |ADS 9706 A (B 9.5m vis, 23deg, 3.6"). d = 0.02P;
TW    Dra |Min II 8.1. P var. Min I = 2433888.452 + 2.806870d*E
TW    Dra |(JD2433000 - 40000) [03825]; since JD2440000 - mean
TW    Dra |elements in the Table.
TX    Dra |Mean magnitude var, P2 = 654d.
UU    Dra |Mean magnitude var, P2 = 960d.
UX    Dra |According to [09086], the light curve may correspond
UX    Dra |to the type E; SB, P ~340d.
UZ    Dra |d = 0.01P; Min II 10.6. Possibly P = 1.65d [03827].
VW    Dra |According to photoelectric observations, 6.28m - 6.32m V.
WW    Dra |Nonlinear term: -4.98d*10**(-9)*E2.
WW    Dra |ADS 10152A (B 9.67m, 8.2", 5deg). Depth of Min II 0.08m.
WZ    Dra |Delta(m) var strongly.
XY    Dra |Min II 13.7.
XZ    Dra |P var. Before JD2438000 Max = 2427985.648 + 0.4764944d*E
XZ    Dra |[00188]. Epochs after JD2438000 are represented dy the
XZ    Dra |elements in the Table only on average. Blazhko effect;
XZ    Dra |according to [01474], Pi = 78d. [Fe/H] = -0.57.
ZZ    Dra |P var. Max = 2434509 + 274.5d*E (JD2416350 - 34600); since
ZZ    Dra |JD2437100 - see Table.
AE    Dra |Delta(S) = (4).
AF    Dra |VR var; SB?
AG    Dra |A soft X-ray source. Elements in the Table represent
AG    Dra |maxima in U band in 1974 - 1979 [09113].
AI    Dra |Min II 7.16, D II = 0.17P.
AP    Dra |Twice shorter period is possible.
AQ    Dra |Hbeta spectral line is probably filled in by emission.
AR    Dra |Min II 11.63.
AS    Dra |mu = 0.486", P = 289deg. SB. Delta(m) var.
AS    Dra |Large spatial velocity. The brightness
AS    Dra |varies with the phase of the orbital motion. Phases
AS    Dra |of Max and Min vary from cycle to cycle. The Table
AS    Dra |gives Porb [03075] and the epoch of the conjunction
AS    Dra |(G4 - star is behind).
AW    Dra |P var. since JD2430500 - see Table.
AX    Dra |Min II 11.0.
BE    Dra |Min II 11.5. The spectral type is late B.
BH    Dra |ADS 12019A (B Am, 9.25m, 10.8", 58deg). Min II 8.58.
BK    Dra |P var.Max = 2415150.817 + 0.592019d*E (JD2414900 - 16150)
BK    Dra |[00001]; since JD2416940 - see Table.
BK    Dra |Delta(S) = 8 in Max light.
BP    Dra |Min II 14.7.
BS    Dra |Min II 9.84.
BV    Dra |ADS 9537 A (B = BW Dra, 16.3", 358deg, 1980; C 12.69m).
BV    Dra |Min II 8.40.
BW    Dra |ADS 9537 B (A = BV Dra; C 12.69m). Min II 9.02.
BY    Dra |SB2 (Porb = 5.9750998d, e = 0.36). mu = 0.365", P = 150deg.
BY    Dra |Quasiperiodic variability :
BY    Dra |DM var, P var, (differential rotation), phase jumps.
BY    Dra |Flares up to Delta(U) = 1.07m.
CM    Dra |VB A (B SP = DC, 15.7m pg, 25.7", 22deg, common mu).
CM    Dra |mu = 1.619", p = 317deg, pi = 0.068", V nu = -118.6km/s.
CM    Dra |Min II 13.63. BY type variability: Delta(M) ~<= 0.05mV,
CM    Dra |P ~Porb. Flares: Delta(m) ~0.05.
CR    Dra |mu = 0.50", p = 168deg, pi = 0.048".
CX    Dra |SB, Porb = 6.69612d (with this period Delta(V) = 0.04m).
CX    Dra |Long-term cyclic variations: P ~2400d, Delta(V) ~0.2m.
CX    Dra |Flares ~0.1m. An X-ray source; the reflection effect is
CX    Dra |observed.
DE    Dra |d = 0.017P.
DG    Dra |Depths respective to Max I (D = 0.25); Min II 0.17m;
DG    Dra |Max II 0.01m.
DK    Dra |Porb = 64.44d.
DK    Dra |Epoch of Min is given. Both components show H and K CaII
DK    Dra |in emission.
DL    Dra |VB A (B 9.2m, 3.9", 318deg, 1982). P1 = 0.0825d, A1 =
DL    Dra |0.028m; P2 = 0.0837d, A2 = 0.026m.
DN    Dra |P = 109S. mu = 0.32", P = 153deg.
kap   Dra |IR excess.
phi   Dra |ADS 11311 (Delta(m) = 1.7m, 0.3", 288deg, 1967). A:SB, P =
phi   Dra |26.768d. The epoch of Max U light is given.
S     Equ |Min II 8.11. P var. Before JD2427000 Min =
S     Equ |2423746.490 + 3.4360050d*E [01140]; Min =
S     Equ |2437968.345 + 3.436072d*E (JD2427000 - 41000)
S     Equ |[03432]; since JD2441000 - see Table.
S     Equ |Gaseous streams; in Min light Halpha is in emission.
W     Equ |Min II 12.4. P var.
Z     Equ |A nearby star: 12.1m.
RT    Equ |P var strongly.
RW    Equ |Strong Blazhko effect.
RZ    Equ |Min II 12.2:.
SU    Equ |Min II 16.4.
SV    Equ |Depth of Min II 0.16m.
SW    Equ |Min II 15.6.
gam   Equ |ADS 14702A (B 11.6m, 2", 268deg; C 12.6m, 48", optical).
gam   Equ |The Table gives the period of oscillations. Data on the
gam   Equ |periodicity of the rotational variability of light,
gam   Equ |spectrum and magnetic field are contradictory
gam   Equ |(17.492d, 314d, 1785.7d, 72yr).
V     Eri |Mean magnitude var, P2 = 1209d.
W     Eri |SiO, OH, H2O maser.
Z     Eri |P2 = 746.4d.
RU    Eri |Min II 9.62.
RX    Eri |[Fe/H] = -1.32.
RY    Eri |d = 0.025P.
RZ    Eri |d = 0.018P. The depth of Min II 0.04m pg.
SV    Eri |[Fe/H] = -1.83. P var. P = 0.71365272d (JD2414000 - 21000);
SV    Eri |P = 0.71370172d (JD2421000 - 26000) [00862];
SV    Eri |Max = 2426590.319 + 0.7137406d*E (JD2426000 -
SV    Eri |34000) [09195]; since JD2434000 - see Table.
TT    Eri |(B - V)Max = +0.255m.
TV    Eri |(B - V)Max = +0.53m.
TZ    Eri |d = 0.015P. P var. Min = 2426066.198 + 2.606097d*E
TZ    Eri |(JD2426000 - 33500) [01490]; since JD2438200 - see Table.
UX    Eri |Min II 11.01. P var? Before JD2438500 Min I =
UX    Eri |2434368.570 + 0.4452820d [02494]; since JD2438500 - see
UX    Eri |Table.
UY    Eri |The shape of the light curve var. [A/H] = -1.6.
VW    Eri |Alternating P1 = 83.4d, P2 = 93.3d. Halo population.
WW    Eri |Min II 11.2.
WX    Eri |The depth of Min II 0.22m. The primary component var,
WX    Eri |DSCT:,  P1 = 0.16454d, P2 = 0.13721d.
YY    Eri |Min II 8.72. P var. Min I = 2433617.5198 + 0.321496212d*E
YY    Eri |(JD2433000 - 41500) [03850]; since 2441500 - see Table.
YY    Eri |X-ray source.
ZZ    Eri |Min II 14.4.
AN    Eri |Min II 14.9.
AO    Eri |d = 0.04P.
AS    Eri |Min II 8.42. X-ray source.
BB    Eri |(k - b)2 = 0.13.
BC    Eri |Min II 11.26:.
BK    Eri |Delta(S) = 8. P var.
BL    Eri |The elements should be checked.
BM    Eri |P > 20000d; D = 321d; d = 270d.
BM    Eri |Only one Min was observed. Outside Min, according to
BM    Eri |[05828], Delta(V) = 0.2m, Max = 2440643.0 + 30d*E.
BQ    Eri |Min II 10.9.
BV    Eri |Min II 8.42. dII = 0.06P.
BW    Eri |Min II 9.72.
BY    Eri |(k - b)2 = 0.06.
BZ    Eri |Min II 9.21.
CC    Eri |SB. mu = 0.310", P = 169deg, Pi = 0.083".
CC    Eri |Photometric P is close to Porb. X-ray source.
CI    Eri |VB (9.9m, 11.2m, 2", 106deg).
CO    Eri |Min II 9.1.
CS    Eri |(k - b)2 = 0.03.
CT    Eri |Min II 10.27.
CW    Eri |Min II 8.86, DII = 0.10P.
DL    Eri |P0 - see Table; P1 = 0.118795d [09206]; P2 = 0.0968d [09207].
DM    Eri |ADS 3380 (5.1m, 5.4m, 0.3", 161deg).
DM    Eri |Duplicity was observed only in 1877 and 1923.
DO    Eri |Epoch of Min is given. Oscillations with P ~6.14 Min, 7
DO    Eri |different frequencies have been found. Beat phenomenon,
DO    Eri |PB = 12.25d +-0.47d. Max of the oscillation amplitude
DO    Eri |almost coincides with Max of the magnetic field, the
DO    Eri |amplitude varies with Prot. Combined amplitude of
DO    Eri |oscillations 0.062m B.
DS    Eri |Min II 10.3. P var. Min = 2423147.25 + 0.827737d*E
DS    Eri |(JD2414869 - 23150); during JD2423150 - 31320 - see Table.
DW    Eri |ADS 3409 B (A 6.72m, G8III; B 9", 317deg).
DY    Eri |ADS 3093 C (A 4.43m V, K1V; B 9.51m V, DA, 82",
DY    Eri |105deg; BC A = 7", Porb = 252.1yr). mu = 4.05", P = 212deg.
DY    Eri |X-ray source.
DZ    Eri |Epoch is given for Max (y), Min (He I).
DZ    Eri |P = 3.67d is possible.
EF    Eri |2A0311 - 227. VB A (B 15.8m, 18", 260deg). mu alpha =
EF    Eri |+0.147", mu delta = -0.070".
EF    Eri |Epoch of narrow Min in IR light is given. The complex
EF    Eri |phenomenon of eclipses is described in [04041].
EF    Eri |Oscillations with P ~20.2 and 13.7 Min. [09211]. Flickering.
EG    Eri |Epoch of Min in Y light is given.
EH    Eri |ADS 3305 A (B 10.8m, 1.45", 60deg, 1917).
HV    Eri |Type RRC: is also possible.
gam   Eri |ADS 2904 A (B 12.4m, 53", 242deg).
lam   Eri |Shell features are sometimes present in the spectrum.
nu    Eri |SB? P2 = 0.1735079d. Beat effect.
omi 1 Eri |P0 - see Table. P1 = 0.1291d.
tau 4 Eri |ADS 2472 A (B 9.9m, 6", 288deg; C 11m, 40", 99deg).
tau 9 Eri |SB1 (Porb = 5.954d). P = 1.2135d is not excluded.
S     For |VB (9.2m, 9.3m, 0.28", 358deg, 1964).
S     For |Found unusually bright only on one night
S     For |by three experienced observers in europe; harvard
S     For |photographs of the same night show it in normal brightness.
V     For |(B - V)Max = +0.26.
W     For |Min II is observed.
RX    For |(k - b)2 = 0.06.
RY    For |(B - V)Max = +0.535.
SS    For |(k - b)2 = 0.09.
SW    For |Delta(S) > 10:.
SY    For |SB2 (M + pec(eq)).
TZ    For |SB2. Possible P values:
TZ    For |37.805d; 44.18d; 50.46d; 75.61d. DI = 1d.
R     Gem |VB A (B 11.4m pg, 173", 200deg, 1910). S 3.5/6e- S 6.5/6-.
S     Gem |VB A (B 11.1m, 70", 122deg).
T     Gem |S 3/4e.
U     Gem |Min = 2437638.82685 + 0.17690602d*E + 5.4d*10**(-12)*E**2
U     Gem |[09215]. Depth of Min 0.5m - 1.0m.
U     Gem |Spectrum description [09216].
V     Gem |P var. Max = 2407750 + 276.2d*E (JD2407700 - 15500);
V     Gem |Max = 2415729 + 278.3d*E (JD2415600 - 21600); Max =
V     Gem |2421839 + 269.8d*E (JD2421700 - 26500) [00458]; Max =
V     Gem |2432580 + 281.3d*E (JD2427500 - 32600); Max =
V     Gem |2434739 + 269.8d*E (JD2432600 - 35800);
V     Gem |since JD2435800 - see Table.
W     Gem |P var. Max = 2429815.990 + 7.914553d*E (JD2413200 -
W     Gem |31700); since JD2431700 - see Table. [A/H] = 0.2.
W     Gem |There is possibly faint blue companion.
RR    Gem |P var. Max = 2415219.734 + 0.39729235d*E
RR    Gem |(JD2412000 - 18000); Max = 2418278.900 + 0.39727274d*E
RR    Gem |(JD2418000 - 21000); Max = 2422865.229 +
RR    Gem |0.39724027d*E (JD2421000 - 25000) [09217]; Max =
RR    Gem |2427150.267 + 0.3972596d*E (JD2426200 - 27850);
RR    Gem |Max = 2434806.289 + 0.3973103d*E (JD2428200 - 34900)
RR    Gem |[02392]; since JD2436000 - see Table. Blazhko effect,
RR    Gem |PB = 48d [03618], PB = 37d [09221]. Delta(S) = 3.
RW    Gem |VB A (B 11.04m, 20", 105deg; C 11.84m, 100", 120deg).
RW    Gem |Min II 9.74; d = 0.02P.
RX    Gem |VB A (B 12.65m, 45", 215deg). Min II 9.28; d = 0.004P.
RX    Gem |P var. Min I = 2417970.0 + 12.20868d*E (JD2415000 - 27500) [07534];
RX    Gem |since JD2427600 - see Table.
RX    Gem |There is a square term in the elements given in the Table:
RX    Gem |+2.25d*10**(-7)*E**2. Luminous gaseous ring surrounds the
RX    Gem |primary component of the system [07535].
RY    Gem |VB A (B 12.30m, 45", 240deg). Min II 8.75; d = 0.023P.
RY    Gem |P var. Min I = 2418015.333 + 9.300876d*E
RY    Gem |(JD2418000 - 33000) [08653]; since JD2433000 - see Table.
RY    Gem |Component of A type is surrounded by a luminous gaseous
RY    Gem |ring.
RZ    Gem |VB. P var. Max = 2429632.453 + 5.529716d*E
RZ    Gem |(JD2415000 - 32400); since JD2432400 - see Table.
SS    Gem |9.9m <= Min II <= 10.7m.
SU    Gem |P var. Min I = 2429204 + 50.12d*E (JD2429200 - 355)
SU    Gem |[00310]; Min I = 2437772.5 + 50.39d*E (JD2437739 -
SU    Gem |39850); Min I = 2439856.6 + 50.10d*E (JD2439850 -
SU    Gem |40680); since JD2440680 - see Table.
SU    Gem |Mean brightness varies with the elements:
SU    Gem |Min = 2437953 + 680d*E; M - m = 264d.
SU    Gem |Amplitude of shortperiodical variations is 0.3m - 0.9m.
SW    Gem |Min brightness epoch is given.
SX    Gem |Min II 11.3; d = 0.05P:.
TX    Gem |Depth of Min II 0.04m; d = 0.017P:.
UV    Gem |VB A (B 19.5m, 7", 285deg).
WW    Gem |Min II 10.3.
WY    Gem |May be an eclipsing system similar to VV Cep. Atmospheric
WY    Gem |eclipse began probably in 1960 - 61, the mean phase of it
WY    Gem |being in 1968 [05730]. Variable magnetic field [01591,04498].
WY    Gem |Intrinsic variability of blue component is also possible
WY    Gem |[07536].
YY    Gem |VB C (A 1.99m, B 2.85m, a = 6.06", P = 306.3 y; C 73",
YY    Gem |165deg, 1925); mu alpha = -0.0154s, mu delta = -0.108".
YY    Gem |Min II 9.59; Min II - Min I = 0.50P; D = 0.000P. X-ray
YY    Gem |source. P const [08655]. Both components are probably
YY    Gem |UV Cet type variables. Flare amplitude in the integrated
YY    Gem |light of the system reaches 0.3m V, or 1.8m U [09227].
AA    Gem |[A/H] = 0.0.
AC    Gem |Min II 11.3. P var. Min I = 2433649.30 + 1.661795d*E
AC    Gem |(JD2415000 - 36000) [01530]; since JD2430100 - see Table.
AF    Gem |VB A (B 14.8m, 2", 0deg). Min II 10.67.
AF    Gem |There is a square term in the elements given in the Table:
AF    Gem |-1.71d*10**(-10)*E**2.
AH    Gem |Min II 14.8:.
AI    Gem |Min II 14.0.
AL    Gem |Min II 9.85.
AN    Gem |Min II 13.3:; d = 0.037P.
AU    Gem |OH emission.
AV    Gem |Min II 12.8:.
AY    Gem |Min II 10.9.
AZ    Gem |Min II 12.4.
BB    Gem |VB A (B 12m, 25", 270deg).
BP    Gem |P var. Max = 2434120 + 243.9d*E (JD2418700 - 36600);
BP    Gem |since JD2436600 - see Table.
BT    Gem |Min II 14.0:.
CI    Gem |UG?
CM    Gem |Min II 15.0.
DL    Gem |VB A (B 13.1m, 18", 180deg).
DN    Gem |VB A (B 13.5m, 12", 16deg; C 12.0m, 80", 99deg).
DP    Gem |Min II 14.0. RRC? P = 0.2792d?
DX    Gem |P var. Max = 2433182.876 + 3.136226d*E (JD2425000 -
DX    Gem |34000); Max = 2435554.199 + 3.136955d*E
DX    Gem |(JD2434000 - 36500) [08300]; since JD2436500 - see Table.
EF    Gem |P var. Min = 2428108.49 + 6.10222d*E (JD2428500 -
EF    Gem |42800) [00407]; since JD2442800 - see Table.
EL    Gem |Min II 13.6.
EN    Gem |Min II 13.8.
EW    Gem |P var. Max = 2428495.686 + 0.523750d*E (JD2428100 - 30780);
EW    Gem |since JD2430780 - see Table.
EY    Gem |Min II 13.0.
FT    Gem |Min II 14.1.
GP    Gem |Min II 13.5.
GR    Gem |15.6 <= Min II <= 15.9.
GW    Gem |Min II 10.68.
GX    Gem |Min II 11.3.
GZ    Gem |P = 1.225290d?
HH    Gem |Min II 13.8.
HR    Gem |Min II 11.7.
HY    Gem |Min II 17.5.
II    Gem |P = 223d?
IP    Gem |Min II 14.5.
IR    Gem |In supermaxima there are superhumps with P = 102 Min
IR    Gem |[09232].
IZ    Gem |D >= 0.24d.
KN    Gem |The minor planet (123) Brunhild.
KQ    Gem |Min II 14.6.
KU    Gem |d = 0.05P.
KV    Gem |Epoch of Min of brightness is given. EW
KV    Gem |type is possible according to the spectrum [09037].
KZ    Gem |The cycle may be 129d.
LM    Gem |d = 0.02P.
LX    Gem |Red.
MO    Gem |Red.
MP    Gem |VB.
MU    Gem |Min II 14.9.
MZ    Gem |Min II 16.7.
NQ    Gem |In the spectrum of the carbon
NQ    Gem |star the hydrogen emission lines and ultraviolet
NQ    Gem |continuous emission appeared in February 1970 [06348].
NY    Gem |HD 47396 (Pec) = S 5438 = CSV 798 = CSV 6468.
NY    Gem |In the chart in [00156] the position of the variable is
NY    Gem |wrong.
OS    Gem |Oscillations with
OS    Gem |the period P1 given in the Table are superimposed
OS    Gem |by oscillations with the period P0 = 0.070d and smaller
OS    Gem |amplitude. P1/P0 = 0.78.
V0345 Gem |The variability may be due to the fainter (B) component.
zet   Gem |VB A (B 11.46m, 87", 84deg; C 7.56m, 97", 350deg). P var.
zet   Gem |Max = 2410640.42 + 10.15477d*E (JD2394600 - 2407150);
zet   Gem |Max = 2422366.187 + 10.15288d*E (JD2407150 - 22300);
zet   Gem |Max = 2426802.918 + 10.15172d*E (JD2422300 - 34500)
zet   Gem |[02392]; since JD2434500 - see Table.
zet   Gem |All the observations are satisfied also by the
zet   Gem |elements: Max = 2443785.444 + 10.150135d*E -
zet   Gem |5.24d*10**(-7)*E**2 [09029].
zet   Gem |May by a DCEPS type variable.
eta   Gem |VB A (B 8.8m, GO III - IV, 1.60", 269.4deg, 1977). SB1
eta   Gem |(P = 2983d [09236]). Epoch of Min brightness is given.
eta   Gem |The deepest minima (corresponding to the middles of the
eta   Gem |descending branches of the radial velocity curve) are
eta   Gem |satisfied by the elements: Min = 2429355 + 2984d*E
eta   Gem |[01551].
mu    Gem |VB A (B 9.8m, 122", 141deg).
sig   Gem |VB A (B 10.8m, 182", 316deg); SB1 (P = 19.603d [09238]).
sig   Gem |There is a Min II on the light curve; Min II sometimes
sig   Gem |disappears and sometimes becomes deeper then Min I.
sig   Gem |Min II - Min I = 0.5P.
U     Gru |Depth of Min II 0.05m. d = 0.011P.
W     Gru |P var. Nonlinear term: +7.84d*10**(-9)*E**2. Min II 10.0.
X     Gru |d = 0.008P. Min II 10.69. P var.
X     Gru |Current elements are given.
Z     Gru |Delta(S) = 12:.
Z     Gru |The shape of the light curve and P are strongly variable.
RS    Gru |(k - b)2 = 0.22.
RT    Gru |(k - b)2 = 0.02. Blazhko effect.
RV    Gru |(B - V)Max = +0.93. Min II 11.4.
RW    Gru |Delta(S) = 10. Blazhko effect.
RX    Gru |Min II 10.7.
RY    Gru |Superposition of irregular variations?
RY    Gru |During JD2434513 - 517 precalculated minima were not
RY    Gru |observed.
RZ    Gru |A description of light changes [02809].
UW    Gru |[Fe/H] = -1.6.
VW    Gru |P >= 260d?
VY    Gru |P > 160d.
VZ    Gru |RR type is also possible.
AK    Gru |Elements should be checked.
AP    Gru |P var. Mean elements JD2427992 - 36848 - see Table.
AP    Gru |during JD2434250 - 36848 Max = 2434337.337 + 0.5082945d*E.
AR    Gru |Min II 10.6.
AV    Gru |P >= 160d is possible.
AW    Gru |Min II? JD2436818.
BC    Gru |Min II 10.3. RRC type is possible.
BD    Gru |Min II 14.9.
BH    Gru |Min II 15.2:.
pi  1 Gru |VB A (B 10.9m, G0V, 2.7", 202deg).
T     Her |VB A (B 10m, 67", 321deg).
U     Her |SiO, OH, H2O maser.
W     Her |ADS 10121 A (B 14.2m, 6", 334deg).
X     Her |P2 = 746d.
Z     Her |VB A (B ro > 10"). Min II 8.18.
Z     Her |nonlinear term: -6.19d*10**(-10)*E**2.
RU    Her |SiO maser. The spectrum in Min
RU    Her |light is composite; a companion? [03502].
RX    Her |Min II 7.74.
SW    Her |B - V; +0.12, +0.40. P var. Before 1921 Max =
SW    Her |2416687.018 + 0.4928864d*E.
SX    Her |[Fe/H] = -1.8.
SY    Her |On period variations see [08699].
SZ    Her |Min II 10.10. P var. Min = 2430766.8390 + 0.818096d*E +
SZ    Her |0.0165d*sin(0.010465deg*E + 180deg) [05749].
SZ    Her |The Table gives current elements satisfac -
SZ    Her |tory after JD2438000.
TT    Her |Min II 9.89. The light curve shape var.
TT    Her |P var. Before JD2430000 Min = 2425433.627 +
TT    Her |0.9120846D [02389]; Min = 2434525.2572 + 0.9120800d*E
TT    Her |(JD2430000 - 40000) [03504]; since JD2440000 - see Table.
TU    Her |d = 0.022P. P var. Before JD2435000 Min =
TU    Her |2424381.416 + 2.2671303d*E - 854d*10**(-11)*E**2 [09240];
TU    Her |Min = 2437462.3909 + 2.2669718d*E (JD2435000 -
TU    Her |38000) [09241]; Min = 2443324.70097 + 2.2669385d*E
TU    Her |(JD2438000 - 44000) [08593]; since JD2444000 - see Table.
TW    Her |[Fe/H] = -0.47.
TX    Her |Min II 8.97, DII = 0.11P. P var;
TX    Her |periodic term: +0.0081d*sin(0.042deg*(E + 7255)).
UU    Her |[Fe/H] = -1.27.
UU    Her |There was alternation of periods 90d and 71d
UU    Her |[00310]; the period 45d [03507] was also noted.
UU    Her |During JD2443611 - 44161 - see Table. Epoch of Min is given.
UX    Her |Min II 9.11. P var. Before JD2429000 Min =
UX    Her |2419876.467 + 1.5488598d*E [00279]; Min =
UX    Her |2429987.420 + 1.5488513d*E (JD2429000 - 38000)
UX    Her |[03671]; since JD2438000 - see Table.
VW    Her |VB A (B 17.3m, 18", 120deg.
VX    Her |Delta(S) = 5. P var; nonlinear term:
VX    Her |-0.00745d (E:10000)**2. According to [03369],
VX    Her |a member of an eclipsing binary system.
VZ    Her |[Fe/H] = -0.9. P var. P = 0.44031880d (JD2415000 -
VZ    Her |22000) [05738]; Max = 2425004.4590 + 0.44032394d*E
VZ    Her |(JD2422000 - 27000); Max = 2425004.4456 +
VZ    Her |0.44032631d*E (JD2427000 - 36000) [03506];
VZ    Her |since JD2436000 - see Table.
WW    Her |VB A (B 15.6m, 7.4", 148.5deg, white).
WX    Her |Twice longer P is not excluded.
AC    Her |P var.
AC    Her |The Table gives current elements valid since JD2442000.
AC    Her |Mean P = 75.4619d [01754]. The magnitude in
AC    Her |Max varies with Delta(m) = 1.6m [00368].
AD    Her |VB A (B 11.97m, 5", 189deg). d = 0.033P. Min II 9.79.
AF    Her |P var. Before JD2426950 P = 0.630336d;
AF    Her |since JD2426950 - see Table.
AF    Her |The shape of the light curve var.
AG    Her |P var. Max = 2422935.584 + 0.6494378d*E
AG    Her |(JD2418210 - 26952); since JD2426952 - see Table.
AH    Her |Porb = 5.9d:. Oscillations during outbursts:
AH    Her |24s <= P <= 39s, Delta(m) <= 0.003m [09251].
AH    Her |Flicckering in Max And Min up to 0.4m in 2 - 8 minutes
AH    Her |[09252].
AK    Her |ADS 10408 A (B 12.0m, 5", 323deg). Min II 8.64.
AK    Her |Min II - Min I = 0.505P. dII = 0.07P. P var. Before
AK    Her |JD2421200 Min = 2421200.549 + 0.42152207d*E; Min =
AK    Her |2421200.549 + 0.42152083d*E (JD2421200 - 24950);
AK    Her |Min = 2424949.555 + 0.42152061d*E  (JD2424950 -
AK    Her |30000) [01760]; Min = 2430939.368 + 0.42152362d*E
AK    Her |(JD2430000 - 41500); since 2441500 - see Table.
AK    Her |The shape of the light curve var.
AM    Her |3U 1809 +50. Lx(soft)/Lopt ~15.
AM    Her |Emissions of H and KCaII, H, HeI, HeII, etc.
AM    Her |In the spectrum. Epoch of Min I in V light is given.
AM    Her |The period shows complex variations. The phase of Min I
AM    Her |in U light is 0.30p, in B 0.15P, in R 0.05P. Min I is
AM    Her |probably due to an eclipse of a hot spot and the gas flow
AM    Her |near the surface of the white dwarf by the white dwarf
AM    Her |itself. The depth of Min I is up to 0.7m. Min II with the
AM    Her |depth up to 0.4m (sometimes absent), Min II - Min I = 0.55P.
AM    Her |Min II coincides  in phase with the X-ray eclipse.
AM    Her |High and low states (b ~13.0m and B ~15.0m on average);
AM    Her |in the high state there are variations with Delta(m) ~0.3m
AM    Her |on the time scale >= 200d; the duration of low states is
AM    Her |130d - 700d [09258] or less. During low states the
AM    Her |depth of minima is small. Flickering up to 0.8mV in
AM    Her |several minutes or dozens of seconds; X-ray flickering
AM    Her |on the time scale of ~10s not correlating with
AM    Her |optical flickering. The magnetic field ~1*10**7 G at
AM    Her |the equator, ~2*10**7 G on poles. Variable circular
AM    Her |(from  +3% to -9%) and linear (up to 7%) polarization.
AM    Her |IR excess at lambda 10 mkm.
AP    Her |P var strongly. P = 10.400d (JD2415000 -
AP    Her |19000:); P = 10.3970d (JD2423700 - 24700:); P =
AP    Her |10.4260d (JD2424700 - 25300); P = 10.4338D
AP    Her |(JD2425800 - 27000); P = 10.3945d (JD2427000 - 27400);
AP    Her |P = 10.4277d (JD2433000 - 33850); P = 10.3898d
AP    Her |(JD2433850 - 34850);  P = 10.4209d (JD2434850 - 35600);
AP    Her |P = 10.3715d (JD2435600 - 37200);
AP    Her |DURING JD2437200 - 43800 - see Table.
AP    Her |The light curve shape var. [A/H] = -0.8.
AR    Her |P var in a complicated way. Max =
AR    Her |2424794.274 + 0.4700234d*E (1905 - 1954) [06535];
AR    Her |Max = 2439692.683 + 0.469975d*E (1954 - 1967) [05274];
AR    Her |since 1967 - see Table.
AR    Her |Blazhko effect, Pi = 31.5489d [03555],
AR    Her |Delta(m) var (0.9m -: 1.8m pg) [02168], (M - m) var.
AR    Her |Delta(S) = 6.
AT    Her |The star is bright on one plate (JD2418209).
AT    Her |Besides that, 11.8m - 12.25m.
AW    Her |VB A (B 10" - 20"). d = 0.03P.
BB    Her |P var. P = 7.507696D (JD2418924 - 30700);
BB    Her |since JD2430700 - see Table. [A/H] = +0.3.
BC    Her |P var. Before JD2432000 Min = 2426242.372 +
BC    Her |3.08752d*E [09262]; since JD2436000 - see Table.
BD    Her |P var. P = 0.4739135d (JD2426540 - 29620); P =
BD    Her |0.4739057d (JD2429620 - 30570); Max = 2430495.404 +
BD    Her |0.4739126d*E (JD2430570 - before 1948) [09263];
BD    Her |since 1948 - see Table. Delta(S) = 0.8.
BL    Her |P var. P = 1.3074604d (JD2415000 - 35000);
BL    Her |since JD2435000 - see Table. Another possible
BL    Her |representation: Max = 2434999.402 + 1.307457d*E -
BL    Her |3.9d*10**(-10)*E**2 (JD2415000 - 42000). [Fe/H] = 0.0.
BO    Her |d = 0.015P. Min II 10.8. P var?
CC    Her |P var. Min = 2426120.415 + 1.7340314d*E (JD
CC    Her |2425790 - 31265); Min = 2431265.288 + 1.7340460d*E
CC    Her |(JD2431265 - 36000) [02389]; Min = 2439668.342 +
CC    Her |1.73398d*E (JD2436000 - 39600); since JD2439600 - see
CC    Her |Table.
CD    Her |The chart in [06286] is wrong.
CE    Her |[A/H] = -1.8.
CK    Her |P var? Max = 2429231.234 + 0.519201d*E (JD2429231 -
CK    Her |877) [00332]; during JD2436041 - 37955 - see Table.
CO    Her |P2 = 600d. Sometimes does not vary for 150d.
CP    Her |Superimposed waves, 50d - 100d.
CT    Her |The depth of min II 0.05m. P var.
CT    Her |Min = 2430904.431 + 1.786337d*E (JD2426480 - 35000)
CT    Her |[03567]; Min = 2439355.666 + 1.7863645d*E
CT    Her |(JD2435000 - 39500) [00001]; Min = JD2441499.3307 +
CT    Her |1.7863891d*E (JD2439500 - 42500) [08593];
CT    Her |since JD2442500 - see Table.
DE    Her |P var. Max = 2425754 + 171.2d*E (JD2425754 - 30890);
DE    Her |Max = 2430889 + 175.3d*E (JD2430890 - 36150);
DE    Her |during JD2436150 - 38140 - see Table.
DF    Her |Elements are valid since JD2425900.
DH    Her |d = 0.024P:. Min II 9.5.
DI    Her |Min II 8.95, DII = 0.03P, Min II - Min I = 0.77P (1966 -
DI    Her |1978). Apsidal motion: P = 29000yr +- 4000yr;
DI    Her |Min II = 2442241.4602 + 10.5501751d*E.
DI    Her |A considerable discrepancy between the observed and
DI    Her |the theoretical rate of apsidal motion.
DK    Her |P var.
DL    Her |Blazhko effect, Pi = 33.6d, 11.0m <= m Max <= 11.3m. P var.
DL    Her |Delta(S) = 5.
DO    Her |Close to V362 Her.
DQ    Her |VB A (B 18.17m, F, 3.5", 132deg, optical?).
DQ    Her |Nebula, R = 10.5" (Halpha, 1981).
DQ    Her |After the main Max of the Nova a deep
DQ    Her |Min 13.0m (JD2426925) and a flat secondary Max
DQ    Her |6.7m (JD2427065) were observed.
DQ    Her |Eclipsing variability:
DQ    Her |14.61m - 18.08m, Min HeI = 2434954.9445 + 0.193620877d*E
DQ    Her |[09280]. D = 0.20P, d = 0.000P.
DQ    Her |The light curve shape and Delta(M) var.
DQ    Her |Oscillations: Max HeI = JED2434954.785868 +
DQ    Her |8.22521640d*10**(-4)*E - 2.8048d*10**(-16)*E**2
DQ    Her |[08722], 0 <= Delta(m) <= 0.08m.
DQ    Her |Polarization changes with double oscilation period.
DQ    Her |Flickering: Delta(m) = 0.15m.
DY    Her |P var, nonlinear term: -18.6d*10**(-13)*E**2.
EI    Her |Red.
EN    Her |P var. Before JD2427000 P = 160d.
ES    Her |Min II 13.7.
ET    Her |The elements are valid earlier than JD2427200
EX    Her |Red.
EZ    Her |The elements are valid earlier than JD2427400.
FN    Her |P var?
FW    Her |Min II 14.6.
FY    Her |According to the spectrum, EW type is possible.
GL    Her |P var?
GU    Her |d = 0.010P. Min II 11.8. Min II - Min I = 0.513P.
GV    Her |[Fe/H] = -1.41. P var. Max = 2427543.360 +
GV    Her |0.2914606d*E (JD2427543 - 29728) [00152];
GV    Her |during JD2436041 - 38170 - see Table.
GY    Her |P var. Max = 2428219.623 + 0.524347d*E (JD2428219 -
GY    Her |727) [00152]; during JD2436370 - 38170 - see Table.
HS    Her |d = 0.025P. Min II 8.63. P var; since JD2438240 - see
HS    Her |Table. Apsidal motion: Pi ~130yr [06538].
HV    Her |d = 0.008P:; Min II 12.9:.
HZ    Her |Her X-1 = 4U 1656 + 35. Lx/Lopt = 2 - 60.
HZ    Her |The Table gives elements for light minima due
HZ    Her |to eclipsing variability and the reflection effect. Min I
HZ    Her |coincides with the X-ray eclipse. Shallow Min II may
HZ    Her |be present. The reflection effect causes variations
HZ    Her |with Delta(m) up to 1.5m. A cycle of 34.875d duration is
HZ    Her |observed in X-ray band; the source is faint during
HZ    Her |two thirds of the cycle. The optical light curve changes
HZ    Her |are observed during the 35d cycle [09283]. According to
HZ    Her |[06539], during JD2427543 - 657 and JD2428630 - 29789 the
HZ    Her |strong reflection effect was absent; the star was still
HZ    Her |varying with P = 1.7d and had Delta(m) ~0.5m,
HZ    Her |Min I = Min II. In [06546] it is stated that
HZ    Her |such intervals with no reflection effect, of 8d to 7a
HZ    Her |duration, took place for almost half the time since
HZ    Her |1890. The light changes during such intervals are in
HZ    Her |the range 14.7m - 15.2m pg. Since 1957 intervals without
HZ    Her |the reflection effect were not observed. In June - July
HZ    Her |1983 the predicted phases of high X-ray flux
HZ    Her |did not take place, but the reflection effect did not
HZ    Her |disappear [09284]. Secondary light variations: P1 =
HZ    Her |1.0977d (delta(B1) = 0.33m), P2 = 0.871173d*E
HZ    Her |(delta(B2) = 0.10m),
HZ    Her |P3 = 1.623846d*E (delta(B3) = 0.17m) [09285]. X-ray pulsar,
HZ    Her |P = 1.2377991s (JD2443357), dP/dt/P = (-2.9 +- 0.2)*10**(-6)/yr
HZ    Her |[09286], sometimes noticeable also in the
HZ    Her |optical range [06543]. Rapid brightness flickering.
IK    Her |d = 0.030P?
IQ    Her |Superposition of variations with shorter P and
IQ    Her |small Delta(m) [06645].
IT    Her |According to the spectrum, EW type is possible.
KL    Her |Min II 14.7.
KV    Her |The light curve is characteristic of Mira Ceti stars
KV    Her |but strongly varies. Many irregularities. O - C: -96d, +73d.
LR    Her |Min II 15.4:.
LS    Her |The light curve shape var.
LT    Her |d = 0.02P. Min II 10.79.
LV    Her |P var? During JD2428429 - 31342 - see Table.
MM    Her |VB A (B 13.50m, 18", 120deg). Min II 9.7.
MM    Her |Delta(m) of the distorsion wave up to 0.12m.
MP    Her |[Fe/H] = -1.18.
MS    Her |Min II 13.3.
MT    Her |Min II 12.30.
MV    Her |The chart in [00156] identifies the variable erroneously;
MV    Her |real MV Her is marked as "C".
MW    Her |P var. P = 503d (1976) [09290]. During
MW    Her |JD24668 - 29172 - see Table.
MX    Her |Moments of Min after JD2444000 published by different
MX    Her |groups of observers contradict each other.
NQ    Her |According to [03882], EA, 8.0 - 8.6 pg, Min II
NQ    Her |8.4, Min I = 2426894.433 + 0.870218d*E (JD2426894 - 34250).
NR    Her |Waves, P = 2.8d - 5.5d.
OQ    Her |Epoch of min is given.
OS    Her |B - V: +0.12,  +0.48.
OU    Her |Spectral type is given according to [02198]; in BSD-G7.
OX    Her |Delta(S) = 6:.
PW    Her |Min II 10.1; DII ~0.3P(!).
V0338 Her |Min II 10.13. P var. Before JD2437000 Min =
V0338 Her |2433771.38 + 1.305732d*E [03115]; Min = 2441864.379 +
V0338 Her |1.3057515d*E (JD2437000 - 43400) [08593,00001];
V0338 Her |since JD2443400 - see Table.
V0342 Her |Min II 10.7.
V0347 Her |P var. Max = 2415288.21 + 0.5373619d*E (JD2415288 -
V0347 Her |18596); since JD2429495 - see Table.
V0359 Her |P var. Min = 2416046.476 + 1.755754d*E (JD2416000 -
V0359 Her |26500) [00001]; Min = 2435693.47 + 1.755775d*E (JD
V0359 Her |2426500 - 36000) [01040]; since JD2443500 - see Table.
V0362 Her |Close to DO Her.
V0365 Her |Blazhko effect: Pi = 40.64d. P var.
V0365 Her |During JD2429037 - 36840 - see Table.
V0373 Her |P = 0.33d or 0.50d is possible.
V0384 Her |P ~0.33d is possible.
V0387 Her |Min II 13.2.
V0394 Her |P var?
V0395 Her |Z = 0.0643.
V0396 Her |Z = 0.175.
V0403 Her |Min II 16.0:.
V0412 Her |Min II 15.2.
V0422 Her |P var? During JD2434131 - 35991 - see Table.
V0423 Her |Min II 15.0.
V0426 Her |Min II 15.8.
V0431 Her |P var.
V0436 Her |The elements are uncertain.
V0441 Her |IR excess, evidence for a circumstellar envelope. Possibly
V0441 Her |non-radial pulsation.
V0442 Her |P var. Max = 2434223.375 + 0.4421143d*E (JD2417447 - 36083);
V0442 Her |since JD2435730 - see Table.
V0442 Her |The shape of the light curve varies.
V0446 Her |Before the outburst 16.2m - 18.8m [03607].
V0451 Her |ADS 10310 A (B 10.70m, 19", 239deg).
V0451 Her |The epoch of Min U light is given.
V0458 Her |[Fe/H] = -1.65.
V0463 Her |P = 54.4d is possible.
V0477 Her |Min II 15.4.
V0482 Her |Possibly eclipsing.
V0499 Her |Blazhko effect.
V0502 Her |Min II 13.5?
V0510 Her |P var?
V0511 Her |P var?
V0513 Her |Min II 15.7.
V0516 Her |Min II 17.1.
V0523 Her |Elements are valid during JD2430940 - 990.
V0524 Her |Twice shorter P is possible.
V0527 Her |Max = 2430938.451 + 0.5188d*E (JD2430938 - 990);
V0527 Her |during JD2436308 - 318 - see Table.
V0529 Her |Epoch of Min is given.
V0529 Her |According to [04217], P = 120d.
V0533 Her |VB A (B 16m, 9.5", 0deg). oscillations:
V0533 Her |Max = 2443717.730281 + 0.0007364941d*E, A ~1% [04162].
V0551 Her |P = 4.00d/n is possible.
V0552 Her |P = 3.04d/n is possible.
V0554 Her |P = 4.01d/n is possible.
V0557 Her |P = 8.00d/n is possible.
V0570 Her |P = 0.5d or 0.33d is possible.
V0578 Her |Red.
V0582 Her |VB. Red.
V0583 Her |Red.
V0588 Her |Possibly eclipsing.
V0600 Her |SB, Porb - see Table. Variability of Vr possibly caused by
V0600 Her |BCEP type pulsations: P - 0.18d.
V0601 Her |Elements are valid since JD2439184.
V0604 Her |Red.
V0608 Her |Blazhko effect.
V0615 Her |Red.
V0618 Her |P var?
V0624 Her |VB A (12.04m, 40"). Min II 6.35. SB2.
V0637 Her |ADS 10227 A (BC 9.2m, 9.2m, 1.7", 18deg, 1975; BC: A =
V0637 Her |0.28", Porb = 56.56yr).
V0639 Her |mu alpha = -0.21", mu delta = +0.39",pi = 0.087".
V0639 Her |VB B (A = V647 Her, 11.36m var, dM4e; B 16", 268deg).
V0639 Her |Flares in the bands U and M pg.
V0640 Her |VB A (B 14.9m, 8.5", 217deg; C 13.9m, 23", 221deg).
V0641 Her |L or ISB type is also possible.
V0644 Her |SB (Porb = 11.859d).
V0645 Her |P ~3h - 10h, a cycle of 40d.
V0647 Her |VB A (B = V639 Her, 16", 268deg); mu alpha = -0.21",
V0647 Her |mu delta = +0.39"; pi = 0.087".
V0652 Her |P var; nonlinear term: -45.80d*10**(-10)*E**2. Delta(m) var.
V0652 Her |Resembles PV TEL type stars but is a helium rich subdwarf.
V0652 Her |Epoch of Max is given. Secondary hump at the phase 0.5P.
V0654 Her |Delta(m) = 0.15m in white light.
V0655 Her |ADS 10407 A (B 9.2m, 4.1", 144deg, 1971).
V0657 Her |According to [02610], CST?, 11.0m.
V0662 Her |Less probable P values: 0.56629d, 0.56710d, 0.56881d,
V0662 Her |0.56970d.
V0685 Her |Min II 15.8.
V0687 Her |Min II 14.9.
V0691 Her |Possible P values: 0.927d, 0.637d.
V0697 Her |H2O, OH maser.
V0699 Her |Min II 16.0:.
V0717 Her |Blazhko effect?
V0718 Her |Min II 14.3.
V0719 Her |EW type with twice longer P is not excluded.
V0720 Her |Blazhko effect?
V0721 Her |Blazhko effect?
V0722 Her |Min II 15.7.
V0723 Her |Min II 15.5.
V0728 Her |Min II 11.4.
V0731 Her |Min II 13.8.
V0731 Her |Twice shorter P is not excluded.
V0732 Her |Min II 13.8.
V0733 Her |Min II 14.3:.
V0737 Her |Blazhko effect?
V0740 Her |Min II 14.4.
V0741 Her |Blazhko effect?
V0742 Her |Min II 14.4.
V0744 Her |Vr var, P = 86.7221d (SB1? nonradial pulsatiob?).
V0744 Her |Rapid spectral variability is possible: P = 2.5552d,
V0744 Her |0.78906d.
V0749 Her |P = 465s.
V0771 Her |Epoch of max U light is given.
V0772 Her |VB AB (7.4m, G0V; 8.5m, G8V:; A = 0.27", E = 0.97, P =
V0772 Her |20.0yr, C 10.62m, 28"). One of the components
V0772 Her |(probably B) is SB1, P = 0.879511d [04056]. The same
V0772 Her |component must be the eclipsing system. Faint X-ray
V0772 Her |source.
V0774 Her |Both flares and "antiflares" (abrupt fadings) of
V0774 Her |comparable amplitude are observed.
V0946 Her |Not Wolf 688, a large-proper-motion star, which is at 17h19m28s.9,
V0946 Her |+33deg05'10" (epoch and equinox 2000.0).
V0973 Her |Suspected rapid brightness variations.
V0994 Her |The secondary component of the double system may also vary.
alf   Her |ADS 10418 A (B 5.39m, 4.9", 107deg, 1973; B - SB2,
alf   Her |G5III + F2V). Slow variations, P ~6yr, Delta(m) ~0.5m;
alf   Her |quicker changes, P ~ 50d - 155d, Delta(m) ~ 0.3m - 1.0m.
alf   Her |Together with the visual companion the
alf   Her |star is surrounded by an enormous envelope (R ~2*10**5R$,
alf   Her |expansion velocity 10 km/s, mass loss 3*10**(-8)M$/yr).
nu    Her |[Fe/H] = -0.26. SB?
omi   Her |VB interferometric.
phi   Her |SB, Porb = 560.5d.
ome   Her |ADS 10054 A (B 11.5m, 0.8", 232deg, 1967; C 11.0m, 28.4",
ome   Her |96deg, 1957; D 27.5", 271deg, 1960). Epoch of Min is given.
ome   Her |Double wave in the light curve.
ome   Her |Rapid variations, P = 0.15d [09310].
g     Her |The mean cycle 1972 - 1981 is given. Slow pulsations
g     Her |(<P> = 875d +- 70d) and non-periodic variations on the
g     Her |time scale of 5d - 15d with Delta(m) up to 0.2m are
g     Her |superimposed.
u     Her |ADS 10449 A (B 10.2m, 4.4", 60deg). Min II 4.93.
R     Hor |OH, H2O, SiO maser. P var. Max = 2428868 + 401.5d*E
R     Hor |(JD2412800 - 28900); since JD2428900 - see Table.
V     Hor |<P> = 59d (JD2428380 - 910), <P> = 90d (JD2429170 - 980).
X     Hor |Epoch of Min brightness is given. Maxima are broad.
X     Hor |Usually secondary minima are observed.
SY    Hor |Min II 12.0.
SZ    Hor |Min II 10.7:.
TU    Hor |Min II 6.03; Min II - Min I = 0.52P;
TU    Hor |Max II is fainter than Max I by 0.05m. Peculiar
TU    Hor |ellipsoidal variable [09245].
TY    Hor |Type RCB?
UU    Hor |P var. Max = 2416826.417 + 0.6436900d*E (JD2416800 - 25000);
UU    Hor |since JD2425000 - see Table.
UX    Hor |Min II 14.4. P var. Min I = 2426659.380 + 0.7126943d*E
UX    Hor |(JD2426650 - 30860); since JD2430540 - see Table.
UZ    Hor |P var. Max = 2426679.425 + 0.338188d*E (JD2426300 - 28430);
UZ    Hor |since JD2430040 - see Table.
VY    Hor |mu = 0.173", ro = 33deg. P = 314s, 617s.
R     Hya |VB A (B 13.0m, 21.6", 324deg). SiO maser. P var. According
R     Hya |to [00458]; Max = 2328201 + 486d*E (JD2328200 - 31120);
R     Hya |Max = 2343512 + 507d*E (JD2343300 - 44800);
R     Hya |Max = 2372678 + 485d*E (JD2372200 - 72700);
R     Hya |Max = 2380447 + 477d*E (JD2380000 - 81400);
R     Hya |Max = 2385160 + 461d*E (JD2384700 - 88000);
R     Hya |Max = 2394350 + 448.6d*E (JD2393900 - 2402000);
R     Hya |Max = 2403742 + 434d*E (JD2403300 - 04200);
R     Hya |Max = 2406363 + 429.5d*E (JD2406000 - 11100);
R     Hya |Max = 2413642 + 411d*E (JD2413200 - 14100);
R     Hya |Max = 2416563 + 405.5d*E (JD2416100 - 23400);
R     Hya |Max = 2424288 + 414.7d*E (JD2423400 - 28500).
R     Hya |since JD2428500 - see Table.
T     Hya |P var. Max = 2399455 + 289.00d*E(JD2398600 - 2421700);
T     Hya |Max = 2422584 + 294.2d*E (JD2421700 - 25800);
T     Hya |Max = 2431781 + 284.20d*E (JD2425800 - 36200); since
T     Hya |JD2437500 - see Table.
V     Hya |VB A (B 11.58mV, KO III, 46", 186deg).
V     Hya |Mean brightness variations with P = 6670d and A = 3.5m are
V     Hya |superimposed by light oscillations with A = 1.1m - 2m and
V     Hya |elements given in the Table. Deep light minima were
V     Hya |observed in 1891, 1908, 1925, 1942 - 43, 1959,  and 1962.
V     Hya |A graph of the light curve [03614].
W     Hya |VB A (B 9.3m, 72", 108deg). P var. Max = 2411074 + 379d*E
W     Hya |(JD2411000 - 14150); Max = 2414644 + 395d*E
W     Hya |(JD2414150 - 19400); Max = 2419746 + 378d*E
W     Hya |(JD2419400 - 25200) [00458]. Max = 2425740 + 366d*E
W     Hya |(JD2425200 - 27000); Max = 2440336 + 397.35d*E
W     Hya |(JD2428000 - 40500); since JD2440500 - see Table.
W     Hya |Amplitude and shape of the light curve vary strongly.
W     Hya |OH, H2O, SiO maser.
X     Hya |OH, H2O, SiO maser.
Y     Hya |Mean magnitude varies.
RR    Hya |H2O maser.
RS    Hya |P var. Max = 2422973 + 330.2d*E (JD2414000 - 23000);
RS    Hya |Max = 2429126 + 342.0d*E (JD2423000 - 29200); Max =
RS    Hya |2429455 + 331.2d*E (JD2429200 - 34500);
RS    Hya |since JD2434500 - see Table.
RT    Hya |Before 1952 <P> = 255d; since 1952 - see Table.
RT    Hya |The character And amplitude of light variations vary
RT    Hya |strongly.
RU    Hya |OH, H2O maser. P var. Max = 2429572 +
RU    Hya |334.0d*E (JD2414000 - 29600); since JD2428500 - see
RU    Hya |Table.
RW    Hya |SB2 (P = 370d). Epoch of Min brightness is given.
RX    Hya |VB A (B 10.5m). Depth of Min II 0.05m. P var.
RX    Hya |Min I = 2428261.385 + 2.2815942d*E (JD2419500 -
RX    Hya |28500); Min I = 2440650.409 + 2.2816200d*E
RX    Hya |(JD2428500 - 41400); since JD2441400 - see Table.
SS    Hya |VB A (B 12.0m, 13", 195deg); SB2.
SU    Hya |Mean magnitude varies with P = 780d.
SV    Hya |VB A (B 35", 225deg). Delta(S) = 7.
SX    Hya |D = 0.022P. P var. Min I = 2427659.223 + 2.895697d*E
SX    Hya |(JD2410000 - 28000) [00007]; since JD2442500 - see Table.
SY    Hya |P var. Min = 2425590.589 + 3.403082d*E (JD2425500 -
SY    Hya |31150) [07548]. Since JD2432200 - see Table.
SZ    Hya |P var. Max = 2415714.1429 + 0.53742815d*E
SZ    Hya |(JD2414700 - 26500) [03626]; Max = 2426410.575 + 0.53736d*E
SZ    Hya |(JD2426400 - 27200) [00001]; Max = 2431881.5537 +
SZ    Hya |0.53723051d*E (JD2427880 - 35200) [03626]; Max =
SZ    Hya |2435542.267 + 0.5372497d*E (JD2435500 - 38900)
SZ    Hya |[03627]. Since JD2438770 - see Table.
SZ    Hya |Blazhko effect: Max(A) = 2440705 + 25.8d*n [06557];
SZ    Hya |10.44m <= Max <= 11.03m.
TT    Hya |Min II 7.32; d = 0.035P.
TU    Hya |P var. Max = 2416980 + 277.5d*E (JD2412500 -
TU    Hya |17300); Max = 2417260 + 272.5d*E (JD2417200 -
TU    Hya |19800) [01787]; Max = 2430410 + 281.4d*E
TU    Hya |(JD2420500 - 30500); Max = 2438332 + 272.3d*E
TU    Hya |(JD2432000 - 39200); since JD2439200 - see Table.
TY    Hya |P var. Min = 2434478.464 + 4.660978d*E (JD2419800 -
TY    Hya |35000) [01788]; since JD2435000 - see Table.
UU    Hya |P var. Max = 2427423.84 + 0.5238585d*E (JD2414950 - 27400)
UU    Hya |[01789]; Max = 2429729.835 + 0.523854d*E (JD2427000 - 31000)
UU    Hya |[00752]. Spectrum is based on Ca II.
UW    Hya |Min II 13.8:; Min II - Min I = 0.64P. P = 1.055439d?
UY    Hya |Min II 13.8. RRC?
VV    Hya |P var. Max = 2427421 + 155d*E (JD2419500 - 37000)
VV    Hya |[01792]; since JD2437000 - see Table.
VX    Hya |(k - b)2 = 0.26.
VX    Hya |Luminosity class [03149] contradicts the type of light
VX    Hya |variability. The shape of the light curve strongly varies.
VX    Hya |The main oscillation with the period P0 given in the Table
VX    Hya |is superimposed by the secondary one with P1 = 0.172720d
VX    Hya |[03631]. P1/P0 = 0.773; Pb = 0.761445d.
VY    Hya |Min II 9.1.
VZ    Hya |Min II 9.46.
WY    Hya |Min II 11.2.
WZ    Hya |(k - b)2 = 0.06. P var. Max = 2416169.681 + 0.53772640d*E
WZ    Hya |(JD2414000 - 19000); Max = 2419811.736 +
WZ    Hya | + 0.53775858d*E (JD2419000 - 21000); Max =
WZ    Hya | = 2424618.630 + 0.53774101d*E (JD2421000 - 32000)
WZ    Hya |[00752]; Max = 2436613.445 + 0.5377229d*E
WZ    Hya |(JD2436600 - 38500) [03633]; since JD2438000 - see Table.
XX    Hya |P var. Max = 2439560.355 + 0.50774868d*E
XX    Hya |(JD2428200 - 39560) [05238]; since JD2439560 - see Table.
XZ    Hya |Min II 15.0.
AE    Hya |Min II 14.6.
AF    Hya |Min II 13.8.
AI    Hya |Min II 9.84; Min II - Min I = 0.438P; DII = 0.075P;
AI    Hya |dI = 0.02P; dII = 0.00P; EA/DM. Pulsation
AI    Hya |period P' = 0.13803d, A = 0.02m - 0.03m [09259].
AV    Hya |Min II 10.35; dI = 0.023P:.
CH    Hya |Min II 15.5; Min II - Min I = 0.57P.
CO    Hya |Found in Lupus, in 10deg to the south from the position
CO    Hya |published by the discoverer [00078].
CW    Hya |P var? [04027].
CW    Hya |Elements given in the Table satisfy observations only in
CW    Hya |the interval JD2428950 - 30375.
DD    Hya |P var. Max = 2431139.313 + 0.501818d*E (JD2431100 -
DD    Hya |600) [01432]. Since JD2441600 - see Table.
DE    Hya |d = 0.014P?
DF    Hya |Min II 11.5.
DH    Hya |Delta(S) = 7.
DK    Hya |Min II 10.7.
DM    Hya |d = 0.15P?
EU    Hya |Min II 10.2.
EX    Hya |Light variations with Porb and amplitude up to 0.9mV
EX    Hya |due to eclipses of hot spot are represented by the
EX    Hya |elements: ET(Min) = 2437699.94177 + 0.0682338422d*E,
EX    Hya |where ET(Min) is the heliocentric Julian Date converted
EX    Hya |to Ephemeris Time; simultaneously periodic modulation of
EX    Hya |the shape of the light curve between the outbursts is
EX    Hya |observed with the amplitude 0.2m - 0.9m and the elements:
EX    Hya |Max = 2437699.8895 + 0.04654656d*E - 1.2d*10**(-12)*E**2
EX    Hya |[09265]. Mean interval between bright outbursts is 465d
EX    Hya |[05695], mean cycle is close to 20 - 30d.
EY    Hya |P var. Max = 2432707 + 160.5d*E (JD2426100 - 32800);
EY    Hya |since JD2432800 - see Table.
EZ    Hya |Min II 10.7. P var. Min I = 2440255.8482 + 0.44976658d*E
EZ    Hya |(JD2431160 - 40650) [07549]; since JD2440250 - see Table.
FG    Hya |Min II 10.25; dI = dII = 0.085P. P var. Min I =
FG    Hya |2431150.388 + 0.3278422d*E (JD2431140 - 34400)
FG    Hya |[00182]; Min I = 2436968.7067 + 0.32783433d*E
FG    Hya |(JD2434050 - 400) [03639]; Min I = 2436968.7067 +
FG    Hya |0.32783546d*E (JD2436950 - 43250) [09267];
FG    Hya |since JD2444600 - see Table.
FI    Hya |V27 in the globular cluster NGC 4590
FI    Hya |(M68); cluster non-member.
FS    Hya |According to [01480] P = 91.7d.
FW    Hya |Min II 12.4.
FY    Hya |VB A (B 15.45m, 15", 90deg); Delta(S) = 7:; (k - b)2 = -0.03.
GK    Hya |Min II 9.57.
GK    Hya |There is a square term in the elements:
GK    Hya |-4.01d*10**(-9)*E**2.
GM    Hya |d <= 0.01P.
GN    Hya |Min II 13.6.
GT    Hya |Cep?
HS    Hya |Min II 8.55.
IK    Hya |Blazhko effect with Pi ~30d.
IW    Hya |OH, H2O maser.
KM    Hya |P var?
KU    Hya |VB AB (7.3m, 7.4m, A = 0.150", P = 58.93 yr, E = 0.219);
KU    Hya |A(v) = 0.06m.
KW    Hya |Porb = 7.75043d; E = 0.110 [09273]; Min II 6.35;
KW    Hya |Min II - Min I = 0.54P.
bet   Hya |VB A (B 5.6m, 0.9", 8deg, 1959).
khi 2 Hya |Min II 5.92.
Y     Hyi |d = 0.024P.
RR    Hyi |In the constellation Octans.
RS    Hyi |In the region of the Small Magellanic Cloud.
RS    Hyi |Not a member of the cloud.
RT    Hyi |Min II 14.1.
RV    Hyi |Min II 12.4; Min II - Min I = 0.61P.
RY    Hyi |In the region of the Small Magellanic Cloud. Not a member
RY    Hyi |of the Cloud.
ST    Hyi |The member of the Small Magellanic Cloud. [A/H] = -0.8.
SZ    Hyi |In the region of the Small Magellanic Cloud. Not a member
SZ    Hyi |of the Cloud.
TW    Hyi |Delta(S) = 10:.
UU    Hyi |P = 112.25d?
VW    Hyi |Mean interval between the supermaxima is 179d.
VW    Hyi |Porb = 0.0742711d. Between the normal outbursts the
VW    Hyi |brightness periodically increases by 0.35m - 0.40m because
VW    Hyi |of hot spot appearances:
VW    Hyi |Max = 2440128.0222 + 0.0742711d*E [07550]. During the
VW    Hyi |supermaxima the period between the superhumps is
VW    Hyi |0.0769d [09275]. Sometimes the light oscillations with
VW    Hyi |the amplitude 2% and cycle from 28s to 34s are observed
VW    Hyi |[07551].
VY    Hyi |In the region of the Small Magellanic Cloud. Not a member
VY    Hyi |of the Cloud.
VZ    Hyi |RR [00193].
WX    Hyi |Mean interval between the supermaxima is 141.5d.
WX    Hyi |Porb = 0.0748134d [09277]. Period between the superhumps
WX    Hyi |observed during the supermaxima is 0.07737d [09278].
WZ    Hyi |In the region of the Small Magellanic Cloud. Not a member
WZ    Hyi |of the Cloud.
ZZ    Hyi |A galaxy PGC 232232 [00001].
AC    Hyi |In the region of the Small Magellanic Cloud. Not a member
AC    Hyi |of the Cloud.
BB    Hyi |Delta(S) = 7:.
V     Ind |P var. Max = 2439792.276 + 0.4796030d*E
V     Ind |(JD2414000 - 40000) [05233]; since JD2440000 - see Table.
V     Ind |Delta(S) = 7, (k - b)2 = 0.02.
RS    Ind |Min II 10.0. P var.
RU    Ind |VB A (B 12.6m, 2.3", 103deg). Min II 12.1.
RX    Ind |240d < P < 310d.
RY    Ind |Min II 11.04.
ST    Ind |Min II 11.79.
SU    Ind |Min II 9.5:.
TV    Ind |Min II 11.9.
AR    Ind |Min II 14.4. RRC?
AY    Ind |mu alpha =  +0.345", mu delta = -0.310"; VB?
R     Lac |VB A (B 14.1m, 6", 50deg).
S     Lac |P var. Max = 2412857 + 238.2d*E (JD2410000 - 16400);
S     Lac |Max = 2418828 + 241.45d*E (JD2416400 - 20500); Max =
S     Lac |2427307 + 242.7d*E (JD2420500 - 27300); Max =
S     Lac |2437290 + 237.4d*E (JD2427300 - 37300);
S     Lac |since JD2437300 - see Table.
U     Lac |There are light variations with the periods:
U     Lac |150d, 550 - 690d, 2900d.
V     Lac |P var. There is a square term in the elements:
V     Lac |-6.48d*10**(-8)*E**2.
W     Lac |P var. Max = 2415255 + 323d*E (JD2414600 - 15300);
W     Lac |Max = 2425628 + 335.5d*E (JD2425600 - 38000) [00458];
W     Lac |Max = 2433844 + 324.5d*E (JD2428000 - 33850);
W     Lac |since JD2433850 - see Table.
X     Lac |P var. Max = 2418890.497 + 5.444303d*E (JD2416670 -
X     Lac |29500) [02033]; since JD2429500 - see Table.
Z     Lac |P var. There is a square term in the elements:
Z     Lac |-3.4d*10**(-8)*E**2. [A/H] = 0.2.
RR    Lac |P var. Max = 2419434.331 + 6.416146d*E (JD2417900 - 31600);
RR    Lac |since JD2431600 - see Table. [A/H] = 0.0.
RT    Lac |Min II 9.62. P var. Min I = 2440382.9005 + 5.0740484d*E +
RT    Lac |1.02d*10**(-8)*E**2 (JD2411650 - 42500) [08592];
RT    Lac |since JD2436470 - see Table.
RT    Lac |There is a square term in the elements given in the Table:
RT    Lac |-2.7d*10**(-8)*E**2. Shape of the light
RT    Lac |curve and depths of the Minima vary. According to
RT    Lac |[09293] the period of the distortion wave migration is
RT    Lac |~9.5 yr, the period of the wave amplitude variations
RT    Lac |(0 < A <= 0.17m) is ~30 yr. According to [09292] the
RT    Lac |migration period is nearly half of the value given in
RT    Lac |[09293].
RV    Lac |Mean magnitude varies with the period 550 - 700d.
RW    Lac |Min II 10.8; DII = 0.024P; Min II - Min I = 0.492P.
RX    Lac |S7.5/1e. P = 174d (JD2414950 - 29550) [01026];
RX    Lac |since JD2436800 - see Table.
RY    Lac |Oscillations of mean magnitude with P = 300 - 420d
RY    Lac |and A <= 0.5m are superimposed by oscillations with
RY    Lac |P = 38 - 91d.
SS    Lac |Probable member of the open cluster NGC 7209. Min II 10.5;
SS    Lac |Min II - Min I = 0.57P; d = 0.008P.
SS    Lac |Apsidal motion with P = 1000 yr is possible.
ST    Lac |Elements should be checked.
SU    Lac |P var. Max = 2412748 + 279.10d*E (JD2412700 - 27000)
SU    Lac |[05707]; Max = 2426972 + 286.74d*E (JD2426900 - 31000);
SU    Lac |Max = 2431008 + 306.0d*E (JD2431000 - 33150)
SU    Lac |[00001]; Max = 2433150 + 319.14d*E (JD2433150 - 42150)
SU    Lac |[05707]; since JD2442100 - see Table.
SW    Lac |Min II 9.31. P var. Min I = 2418943.712 + 0.32071236d*E
SW    Lac |(JD2410000 - 19990); Min I = 2420038.621 +
SW    Lac |0.32071510d*E (JD2419990 - 25210); Min I =
SW    Lac |2430996.525 + 0.32071665d*E (JD2425210 - 33690);
SW    Lac |Min I = 2436046.5634 + 0.32072132d*E (JD2433690 - 36755)
SW    Lac |[05222]; Min I = 2437572.5723 + 0.32072811d*E
SW    Lac |(JD2436755 - 40000) [03374]; Min I = 2440467.4592 +
SW    Lac |0.32072480d*E (JD2440110 - 40500) [06089]; Min I =
SW    Lac |2441249.3737 + 0.3207197d*E (JD2440500 - 41600);
SW    Lac |[00001]; Min I = 2442697.4039 + 0.3207144d*E
SW    Lac |(JD2441600 - 43100) [09295]; Min I = 2443459.7476 +
SW    Lac |0.3207216d*E (JD2443100 - 44400) [09297]; Min I =
SW    Lac |2444856.8064 + 0.3207184d*E (JD2444400 - 44900)
SW    Lac |[00001]; since JD2444900 - see Table.
SW    Lac |Shape of the light curve, depths of minima and heights
SW    Lac |of maxima vary.
TW    Lac |d = 0.018P. P var. Min I = 2424387.332 + 3.0374936d*E
TW    Lac |(JD2424380 - 34000) [02389]; Min I = 2434049.593 +
TW    Lac |3.037520d*E (JD2434000 - 36560) [03115];
TW    Lac |since JD2441500 - see Table.
TZ    Lac |In the region of the open cluster NGC 7243.
UW    Lac |Depth of Min II 0.05m; d = 0.028P. P var.
UW    Lac |Min I = 2429158.17 + 5.2902d*E (JD2414580 - 29440)
UW    Lac |[01813]; Min I = 2429158.17 + 5.290000d*E
UW    Lac |(JD2429440 - 35800) [03115]; since JD2436800 - see Table.
UW    Lac |Apsidal motion is possible [09300].
UY    Lac |d = 0.022P.
UZ    Lac |P var?
VX    Lac |P var. Min = 2424791.488 + 1.0744891d*E
VX    Lac |(JD2424700 - 32400); Min = 2432479.477 + 1.0744991d*E
VX    Lac |(JD2432400 - 40510); Min = 2440750.971 +
VX    Lac |1.0744881d*E (JD2440750 - 43000) [07552];
VX    Lac |since JD2443000 - see Table.
VY    Lac |Min II 10.6. P var? Min I = 2434629.392 + 1.036245d*E
VY    Lac |(JD2424700 - 39830) [01804]; since JD2440080 - see Table.
WY    Lac |Light variations with P = 850d and A = 1.5m are
WY    Lac |superimposed by variations with P = 50d and A = 1m.
XX    Lac |In the region of the open cluster NGC 7243.
XZ    Lac |P var.
AG    Lac |Min II 14.0.
AR    Lac |Min II 6.43; Min II - Min I = 0.5018P; dI = 0.045P; DII =
AR    Lac |0.13P; dII = 0.00P. P var. Min I = 2426624.378 +
AR    Lac |1.983244d*E (JD2415300 - 26800) [09309]; Min I =
AR    Lac |2429535.739 + 1.9832125d*E (JD2426800 - 36000)
AR    Lac |[09312]; Min I = 2437018.414 + 1.983252d*E
AR    Lac |(JD2436000 - 37500) [00001]; since JD2437500 - see Table.
AR    Lac |There is a square term in the elements
AR    Lac |given in the Table:  - 5.24d*10**(-9)*E**2.
AR    Lac |Shape of the light curve varies; there is a
AR    Lac |distortion wave with A up to 0.13mV migrating in the
AR    Lac |direction of decreasing phases with P ~2.5 yr. Spectrum
AR    Lac |investigations [01816,09315,9316].
AU    Lac |Min II 12.2; Min II - Min I = 0.53P.
AW    Lac |Min II 11.2.
BH    Lac |Hydrogen lines in the spectrum are sharp and deep [03149].
BL    Lac |Z = 0.07; <B-V> =  +1.0. Light curve graph [06784].
BM    Lac |The elements are valid in the interval JD2425200 - 26250.
BT    Lac |There is a square term in the elements: -0.0004d*E**2.
BT    Lac |Epoch of Max brightness is given in the Table.
BT    Lac |Mean brightness varies in the range 13.8m - 15.2m with
BT    Lac |P = 654d. Mean amplitude of the shortperiodical variations
BT    Lac |is ~1.5m. There occur changes of primaries and
BT    Lac |secondaries minima into each other.
BU    Lac |The main variation is superimposed by waves with a
BU    Lac |possible period -200d.
CG    Lac |Min II 14.0.
CM    Lac |Min II 8.53; DII = 0.12P.
CN    Lac |Min II 12.6. In the region of the
CN    Lac |open cluster NGC 7209. Not member of the cluster.
CO    Lac |Min II 10.79. Apsidal motion with
CO    Lac |P = 42.3 yr is observed. There is a periodic term in
CO    Lac |The elements given in the Table: -0.0133d cos(157.7deg +
CO    Lac |0.0359deg*E). Min II = 2427534.8439 + 1.5422075d*E +
CO    Lac |0.0133d cos(157.7deg + 0.0359deg*E).
CS    Lac |Min II 9.4.
CZ    Lac |Delta(S) = 1. P var. Max = 2432878.234 + 0.43210346d*E
CZ    Lac |(JD2428700 - 39400) [01442]; Max = 2443081.309 +
CZ    Lac |0.4319850d*E (JD2439400 - 43100) [05839]; Max =
CZ    Lac |2444080.122 + 0.432114d*E (JD2443800 - 44100)
CZ    Lac |[09009]; since JD2445100 - see Table.
DD    Lac |VB A (B 9.2m, 69", 16deg).  P var. Max = 2421914.178 +
DD    Lac |0.19309018d*E - 0.001798d*10**(-8)*E**2 (JD2421400 -
DD    Lac |37600) [05711]; since JD2443000 - see Table.
DD    Lac |According to [09337] simultaneously the pulsations with
DD    Lac |the following periods are observed (the corresponding AB
DD    Lac |values are given in the brackets): P1 = 0.193082d (0.080m),
DD    Lac |P2 = 0.197382d (0.034m), P3 = 0.182115d (0.020m),
DD    Lac |P4 = 0.187438d (0.016m), P5 = 0.095109d (0.010m),
DD    Lac |P6 = 0.23583d (0.008m). A var; 0.04m <= A <= 0.12m.
DE    Lac |Delta(S) = 5. P var. Max = 2428807.130 + 0.2536940d*E
DE    Lac |(JD2427000 - 33000); Max = 2433005.766 + 0.2536929d*E
DE    Lac |(JD2433000 - 39100) [03378]; since JD2442000 - see Table.
DF    Lac |[A/H] = 0.2.
DG    Lac |P var. Min = 2426266.355 + 2.206435d*E (JD2426200 - 40000)
DG    Lac |[04961]; since JD2440000 - see Table.
DH    Lac |P var. Max = 2418240 + 284.8d*E (JD2418000 - 27350);
DH    Lac |since JD2427300 - see Table.
DM    Lac |Erroneously labeled VV306, instead of VV307, in the chart [05862].
DO    Lac |According to [00085], EA.
EG    Lac |P > 50d? [05386].
EM    Lac |Min II 13.09.
EN    Lac |VB A (B 11.32mV, 27", 345deg; C 9.0mV, 62", 48deg); SB1
EN    Lac |(Porb = 12.0968d). Eclipsing system with a pulsating
EN    Lac |primary component of BCEP type. Depth of Min I 0.05mB.
EN    Lac |Min I = 2444909.4339 + 12.096816d*E; D = 0.015P,
EN    Lac |d = 0.000P. Simultaneously pulsations are
EN    Lac |observed with the periods P1 = 0.169170d, P2 = 0.170770d,
EN    Lac |P3 = 0.181692d [09346]. The corresponding amplitudes
EN    Lac |of pulsations vary. The values of the amplitudes in
EN    Lac |B system are as follows: A1 = 0.046m, A2 = 0.024m,
EN    Lac |A3 = 0.022m (1952 - 1965); A1 = 0.016m, A2 = 0.010m,
EN    Lac |A3 = 0.014m (1977); A1 = 0.010m, A2 = 0.014m, A3 = 0.023m
EN    Lac |(1980 - 81). 0.01m <= A <= 0.11m.
EO    Lac |Min II 12.9; Min II - Min I = 0.485P.
EP    Lac |Depth of Min II 0.04m.
ER    Lac |Depth of Min II 0.05m:.
ES    Lac |Min II 11.6; Min II - Min I = 0.57P.
ES    Lac |Apsidal motion is possible:
ES    Lac |Min II = 2433582.95 + 4.459451d*E [09347].
EU    Lac |The chart in [05862] is wrong.
EV    Lac |VB A (B 12.74mB, 10", 260deg, 1949); mu alpha = -0.065s,
EV    Lac |mu delta = -0.46". Dark companion (A = 0.0206", P = 45 yr,
EV    Lac |E = 0.5) [09348]. In 1979 sinusoidal light oscillations
EV    Lac |were observed in the range 10.20m - 10.27mV:
EV    Lac |Min = 2444037.576 + 4.378d*E [09349]. In 1974 - 76 such
EV    Lac |periodicity was not observed [09350].
EW    Lac |Non-radial pulsations with P = 0.7d - 0.8d
EW    Lac |are also possible [09351,09352].
EX    Lac |d = 0.050P.
FQ    Lac |A var; P var. Elements given in the Table are valid in the
FQ    Lac |intervale JD2427950 - 31700.
FU    Lac |d = 0.013P.
GS    Lac |Min II 15.2.
GX    Lac |Min II 10.23.
HK    Lac |SB1 (Porb = 24.4284d [09355]).
HM    Lac |Depth of Min II 0.05m.
HN    Lac |Min II 14.7.
HQ    Lac |Erroneously labeled VV307, instead of VV306, in the chart [05862].
HR    Lac |Min II 14.3.
HT    Lac |In the region of the open cluster NGC 7209.
HW    Lac |Min II 14.8.
HX    Lac |Min II 14.8.
HZ    Lac |Min II 15.0.
IM    Lac |Min II 13.2.
IN    Lac |E?
IP    Lac |Min II 14.0.
IR    Lac |Min II 15.4; d = 0.03P.
IT    Lac |P var.
IU    Lac |Min II 13.5.
IY    Lac |Blazhko effect?
IZ    Lac |Min II 12.7.
KO    Lac |Min II 14.7.
KP    Lac |P < 1d.
KR    Lac |Min II 15.8; dII = 0.05P.
KS    Lac |Depth of Min II 0.03m.
KU    Lac |Depth of Min II 0.03m.
LU    Lac |Min II 15.32.
LW    Lac |d = 0.03P. Depth of Min II 0.03m?
LY    Lac |Min II 12.6.
LZ    Lac |Min II 12.5.
MO    Lac |d = 0.04P. Depth of Min II 0.05m.
MP    Lac |Min II 12.5.
MV    Lac |Min II 15.0.
MZ    Lac |Min II 12.1; Min II - Min I = 0.713P.
MZ    Lac |Min II = 2433872.702 + 3.158719d*E. Elements for Min I
MZ    Lac |are given in the Table.
NN    Lac |d = 0.02P. np (usually brighter) component of a close pair.
NN    Lac |The range of combined brightness is given in the Table.
NO    Lac |Depth of Min II 0.03m.
NR    Lac |Min II 13.4. Sp (brighter) component of a close pair. The
NR    Lac |range of combined brightness is given in the Table.
NU    Lac |EW?
NW    Lac |Min II 13.9. Close binary, the components of which are
NW    Lac |equal in brightness at minimum light. The range of
NW    Lac |combined brightness is given in the Table.
OO    Lac |Min II 12.8.
OV    Lac |150d <= P <= 200d.
OX    Lac |Depth of Min II 0.04m.
PP    Lac |Min II 12.0.
PT    Lac |Min II 15.4.
PZ    Lac |In the region of the open cluster NGC 7243.
QQ    Lac |In the region of the open cluster NGC 7243.
QU    Lac |Depth of Min II 0.04m.
V0335 Lac |Min II 15.8.
V0338 Lac |In the region of the open cluster IC 1434.
V0339 Lac |P = 3.4084964d?
V0340 Lac |Min II 12.4; Min II - Min I = 0.762P;
V0340 Lac |Min II = 2432858.521 + 19.943102d*E.
V0340 Lac |Elements for Min I are given in the Table.
V0342 Lac |Min II 12.9.
V0343 Lac |Min II - Min I = 0.57P. Depth of Min II 0.03m:.
V0344 Lac |Min II 13.0. Min I = 2433873.5784 + 0.39222768d*E
V0344 Lac |(JD2432800 - 35800); since JD2445200 - see Table.
V0345 Lac |Min II 11.6; Min II - Min I = 0.340P; DII = 0.040P;
V0345 Lac |dII = 0.014P. Apsidal motion is possible.
V0347 Lac |VB.
V0350 Lac |VB A (B 9.7m, 66", 94deg); SB1 (P = 17.755d [09356]).
V0350 Lac |Min II 6.45 [07468]. Mean magnitude varies. See also [08933].
V0355 Lac |Northern component of a pair.
V0360 Lac |SB2 (P = 10d [09357]). Min II 5.93.
V0362 Lac |VB A (B 13.2m, 1.8", 49deg).
V0363 Lac |VB A (B 11.3m, F6 III - V:, 6.3", 325deg).
V0364 Lac |Min II 9.15; Min II - Min I = 0.52P; dI = 0.003P,
V0364 Lac |DII = 0.077P, dII = 0.009P.
V0412 Lac |SB, Porb = 41.95yr.
V0413 Lac |SB, Porb = 2.9833d.
V0442 Lac |Quasi-periodic brightness variations of a planetary nebula, possibly
V0442 Lac |due to variable mass loss or pulsations.
R     Leo |P var. Max = 2385112 + 312.43d*E (JD2385100 - 2402500);
R     Leo |Max = 2402929 + 314.33d*E (JD2402500 - 11500);
R     Leo |Max = 2411416 + 308.93d*E (JD2411500 - 16500);
R     Leo |Max = 2416984 + 317.84d*E (JD2416500 - 22500);
R     Leo |Max = 2423328 + 312.75d*E (JD2422500 - 27000);
R     Leo |Max = 2427081 + 307.40d*E (JD2427000 - 30000);
R     Leo |Max = 2437337 + 312.13d*E (JD2430000 - 37500);
R     Leo |since JD2437500 - see Table. SiO, H2O, OH maser.
S     Leo |P var. Max = 2420654 + 189.24d*E (JD2420200 - 26100);
S     Leo |Max = 2426142 + 185.92d*E (JD2426100 - 28100);
S     Leo |since JD2428100 - see Table.
T     Leo |SB1 (Porb = 0.05881873d [09304]).
V     Leo |H2O maser.
W     Leo |P var. Max = 2434651 + 385.41d*E (JD2409500 - 35000);
W     Leo |since JD2437500 - see Table. OH maser.
Y     Leo |P var. Min = 2422372.520 + 1.6860978d*E (JD2418000 - 23500)
Y     Leo |[02389]; Min = 2422372.5368 + 1.68607314d*E
Y     Leo |(JD2423500 - 38600) [09307]; since JD2438600 - see Table.
Y     Leo |There is periodic term in the elements given in the Table:
Y     Leo |+0.00375d*sin(0.21487deg*E + 141.7deg). Depth of Min II
Y     Leo |0.1m IR.
RR    Leo |Delta(S) = 7.1. P var. Max = 2430440.3385 + 0.45238172d*E +
RR    Leo |1.963d*10**(-10)*E**2 (1898 - 1977) [08299]; since
RR    Leo |JD2441400 - see Table.
RT    Leo |Min II 10.5.
RW    Leo |P var. Before JD2440800 Min = 2424993.458 +
RW    Leo |1.6825365d*E [03115]; since JD2440800 - see Table.
RX    Leo |Delta(S) = 6.8.
SS    Leo |P var. Max = 2415485.723 + 0.62633242d*E
SS    Leo |(JD2414000 - 22000) [00752]; since JD2422000 - see Table.
SS    Leo |[Fe/H] = -1.59.
ST    Leo |(k - b)2 = 0.08.
SZ    Leo |P var. Before JD2442500 Max = 2425331.400 +
SZ    Leo |0.5340833d*E [04157]; since JD2442500 - see Table.
SZ    Leo |Light curve shape var?
TV    Leo |P var. Max = 2419852.318 + 0.6728362d*E
TV    Leo |(JD2419000 - 28000) [00001]; since JD2437000 - see Table.
TV    Leo |(k - b)2 = -0.01.
TX    Leo |VB A (B 7.8m, 2", 157deg, 1971);
TX    Leo |A binary according to lunar occultation data: ro = 0.0005".
TX    Leo |The range of combined brightness is given.
TX    Leo |Min II 5.69; DII = 0.19P; Min II - Min I = 0.550P.
TY    Leo |Elements need confirmation.
TU    Leo |Minor planet (8) Flora.
UU    Leo |Min II 11.5. P var. Since JD2430000 - see Table.
UV    Leo |Min II 9.49; d = 0P014. P var. Before JD2434000
UV    Leo |Min I = 2425574.302 + 0.60008516d*E [07554];
UV    Leo |since JD2434000 - see Table.
UX    Leo |Min II 10.4.
UX    Leo |Moments of Min by BBSAG contradict the tabulated elements.
UZ    Leo |Min II 10.12. P var, nonlinear term: +2.8d*10**(-12)*E**2.
XX    Leo |Min II 11.4. Period should be checked.
XY    Leo |Min II 9.80. P var. Min = 2435195.66306 + 0.2841091d*E
XY    Leo |(JD2434000 - 36500) [03392]; Min = 2437376.465 +
XY    Leo |0.28409592d*E (JD2436500 - 40000) [00001]; Min =
XY    Leo |2441005.5364 + 0.28410727d*E (JD2441000 - 44000)
XY    Leo |[09084]; since JD2444000 - see Table.
XY    Leo |The light curve shape var.
XZ    Leo |Min II 11.1.
AB    Leo |Epoch of Min is given.
AB    Leo |According to [01853], Max = 2428880 +
AB    Leo |103.2d*E (JD2414600 - 19000, 2428000 - 31600);
AB    Leo |During other time intervals cycles 75d - 125d.
AD    Leo |mu = 0.49", P = 265deg; pi = 0.20".
AD    Leo |X-ray and radio source. Astrometric binary?
AF    Leo |H2O maser.
AM    Leo |VB A (B 10.64m, 11", 270deg). Min II 9.83.
AP    Leo |Min II 9.88. P var. Min = 2414986.868 + 0.430350d*E
AP    Leo |(JD2414700 - 18600); since JD2418600 - see Table.
AP    Leo |Light curve shape var.
AQ    Leo |Elements for fundamental mode pulsations (P0) see Table.
AQ    Leo |For the first overtone: P1 var?;
AQ    Leo |P1 = 0.4101369d (1929 - 1969); P1 = 0.410130d (1957 -
AQ    Leo |1969); during 1973 - 1975 Max1 =
AQ    Leo |2441766.486 + 0.4101487d*E. delta(M0) = 0.23m,
AQ    Leo |delta(M1) = 0.46M.
AU    Leo |Vr = +7545 km/s. Variability is doubtful.
BB    Leo |[Fe/H] = -1.32.
BL    Leo |Min II14.4. P var. Since JD2442000 - see Table.
BV    Leo |Min II 16.1.
BW    Leo |Min II 15.4.
BX    Leo |[Fe/H] = -1.23.
BZ    Leo |Min II 15.8.
CD    Leo |Light curve shape var.
CE    Leo |Min II 12.5. P var?
CE    Leo |Min by BBSAG contradict the tabulated elements.
CN    Leo |Mu = 4.7", P = 235deg; pi = 0.41".
CN    Leo |Soft X-ray source, radio source.
CW    Leo |Dust envelope, 6"*4".
CW    Leo |Molecular radioemission: SiO, SiS, HCN, HC3N, CO, H2O,
CW    Leo |NH3, etc. Polarization in I band up to 24%.
CX    Leo |VB A (B 12.3m, 132deg); SB (Porb = 12685.4d).
CY    Leo |mu = 0.307", P = 141.3deg; pi = 0.022".
CY    Leo |Outside flares Delta(m) < = 0.036m; P = 600s, 822s, 1638s
CY    Leo |[06209]. A single strong flare with delta(M) = 0.61m in
CY    Leo |blue light of 10 Min duration was observed [06141],
CY    Leo |which is attributed by several authors to the presence of
CY    Leo |a red flaring companion.
DE    Leo |P = 1.2d - 2.0d?
DG    Leo |VB B (A 6.6m, A 8IV, SB2, Porb = 4.15d; B 6.9m, 0.271",
DG    Leo |211.2deg, 1980, Porb ~200yr).
DG    Leo |The range of the bombined brightness is given.
DH    Leo |SB1, Porb = 1.070354d.
DK    Leo |mu alpha = -0.097", mu delta = -0.214".
FL    Leo |Variability range according to E.M. Halbedel, IBVS No. 3502, 1990.
FX    Leo |Not a nearby star (despite having a Gl number).
R     LMi |SiO, H2O, OH mazer.
T     LMi |Min II 10.97. P var. Min I = 2420573.698 + 3.019889d*E
T     LMi |(JD2420200 - 25000); Min I = 2423856.323 +
T     LMi |3.0199336d*E (JD2423800 - 35500); since JD2438400 - see
T     LMi |Table.
U     LMi |1m <= A <= 3.3m. Periodicity sometimes breaks down.
V     LMi |Delta(S) = 5.7.
Y     LMi |P var. Max = 2428636.322 + 0.52443938d*E + 0.0597d*
Y     LMi |*sin(0.0657deg*E + 27.2deg) (JD2425250 - 28500); Max =
Y     LMi |2428636.348 + 0.5244564d*E (JD2428500 - 30000)
Y     LMi |[01856]; mean elements
Y     LMi |for interval JD2432200 - 38900 are given in the
Y     LMi |Table; in this interval the period changed with the
Y     LMi |cycle of ~2100d. Blazhko effect with the period 33.4d
Y     LMi |[01856]; 07m <= A <= 1.9m, 0.19P <= m - M <= 0.44P.
RT    LMi |Min II 11.7.
RU    LMi |Spectrum description [09326].
RW    LMi |VB A (B 15.5m B, 9", 10deg). 0.3m - 2.6m K, 7.64m - 10.71m,
RW    LMi |9.7m - 14.6m R, 14.1m - 18.1m B, 14.8m - 18.6m U.
RW    LMi |Mean brightness varies. Gaseous-dust circumstellar
RW    LMi |envelope. CO emission. Spectrum description [09327].
RY    LMi |VB A (B 16.1m, dM2, 15", 126deg); mu = 0.14", P = 264deg.
RY    LMi |P0 = 215.197388s, dP0/dt = 5.6s*10**(-14)/s, A0 = 0.0440m;
RY    LMi |P1 = 304.4s, A1 = 0.0150m; P2 = 271.0s, A2 = 0.0134m;
RY    LMi |P3 = 107.6s, A3 = 0.0032m; P4 = 126.2s, A4 = 0.0028m;
RY    LMi |P5 = 119.8s, A5 = 0.0026m.
RY    LMi |Mean brightness varies by 0.05m.
R     Lep |P var. Max = 2398883 + 436.44d*E (JD2398000 - 2412000);
R     Lep |Max = 2412849 + 418.04d*E (JD2412000 - 23000);
R     Lep |Max = 2423300 + 441.38d*E (JD2423000 - 36000);
R     Lep |since JD2436000 - see Table.
R     Lep |A var; 5.5m <= Max <= 9.5m (Possible period is more
R     Lep |than 40 years [03402]).
S     Lep |Mean magnitude varies with the cycle of 890d. H2O maser.
T     Lep |SiO maser.
U     Lep |P var. Max = 2425084.431 + 0.58147098d*E
U     Lep |(JD2411000 - 25090); Max = 2425084.431 + 0.58147377d*E
U     Lep |(JD2425080 - 37700) [03403]; since JD2436600 - see Table.
U     Lep |Delta(S) = 8.5; (k - b)2 = 0.00.
V     Lep |Min II 9.9.
Z     Lep |Min II 12.0:.
RR    Lep |Min II 10.4.
RS    Lep |Min II 9.96.
RU    Lep |P var?
RZ    Lep |S 4/4.
SS    Lep |SB2 (Porb = 258.2d [09363]).
SY    Lep |VB A (B 15.2m: V, 18", 270deg).
S     Lib |P var. Max = 2405692 + 192.14d*E (JD2402700 - 24000);
S     Lib |Max = 2424141 + 194.74d*E (JD2424000 - 30500);
S     Lib |Max = 2431900 + 190.34d*E (JD2430500 - 37200);
S     Lib |Max = 2439203 + 197.61d*E (JD2437200 - 39300);
S     Lib |since JD2441000 - see Table. Mean value of the period is
S     Lib |given in the Table. A var (1.8m <= A <= 5m).
W     Lib |P var. Max = 2412272 + 203.76d*E (JD2412000 - 28500);
W     Lib |Max = 2428573 + 201.48d*E (JD2428500 - 34000);
W     Lib |since JD2434000 - see Table.
X     Lib |P var. Max = 2423500 + 165.75d*E (JD2413000 - 25000);
X     Lib |since JD2425000 - see Table.
Y     Lib |P var. Max = 2413452 + 275.7d*E (JD2413400 - 22000);
Y     Lib |Max = 2422273 + 272.5d*E (JD2422000 - 28000) [00458];
Y     Lib |Max = 2434921 + 277.04d*E (JD2428000 - 35000);
Y     Lib |since JD2435000 - see Table.
Z     Lib |P var. Max = 2417736 + 294.5d*E (JD2407100 - 17800);
Z     Lib |since JD2424400 - see Table.
RR    Lib |P var. Max = 2409699 + 277.4d*E (JD2409600 - 15600);
RR    Lib |Max = 2416345 + 273.2d*E (JD2416300 - 19700);
RR    Lib |Max = 2421027 + 278.6d*E (JD2421000 - 27150) [00458];
RR    Lib |since JD2427150 - see Table.
RS    Lib |P var. Max = 2413396 + 217.2d*E (JD2413300 - 20000);
RS    Lib |Max = 2420110 + 219.6d*E (JD2420000 - 27500) [00458];
RS    Lib |Max = 2429078 + 215.6d*E (JD2427500 - 35000);
RS    Lib |Max = 2438196 + 219.9d*E (JD2435000 - 42600);
RS    Lib |since JD2441700 - see Table.
RT    Lib |P var. Max = 2413776 + 254.21d*E (JD2413000 - 19000);
RT    Lib |since JD2419000 - see Table.
RU    Lib |P var. Max = 2413363 + 312.0d*E (JD2413300 - 16200);
RU    Lib |Max = 2416807 + 322.5d*E (JD2416800 - 21000);
RU    Lib |Max = 2421309 + 317.0d*E (JD2421300 - 24200);
RU    Lib |Max = 2424804 + 311.5d*E (JD2424800 - 29800) [00458];
RU    Lib |Max = 2434909 + 319.9d*E (JD2429800 - 35000); since
RU    Lib |JD2437700 - see Table.
RV    Lib |Min II 9.44.
RX    Lib |[A/H] =  -0.5. P var. Max = 2430913.6 + 24.950d*E
RX    Lib |(JD2425000 - 36300) [00266]; since JD2436300 - see Table.
SS    Lib |Min II 10.8; d = 0.030P.
ST    Lib |VB A (B 14m, 14", 0deg).
TV    Lib |Delta(S) = 2.5.
TY    Lib |d = 0.019P.
UW    Lib |[Fe/H] =  - 0.25.
VV    Lib |P var. Max = 2424268.474 + 0.4781418d*E
VV    Lib |(JD2419800 - 2425000); since JD2425000 - see Table.
VW    Lib |Observations given in
VW    Lib |[00293] contradict the elements given in the Table.
VY    Lib |P var? [03506].Delta(S) = 6.
VZ    Lib |Min II 10.55; dI = 0.000P; dII = 0.005P. P var. Min I =
VZ    Lib |2429022.227 + 0.358053d*E (JD2428600 - 30400)
VZ    Lib |[09368]; Min I = 2430899.223 + 0.358448d*E
VZ    Lib |(JD2430400 - 32400) [02532]; since JD2444330 - see Table.
YZ    Lib |Min II 12.9.
AA    Lib |P var? The elements are valid in the interval
AA    Lib |JD2427800 - 29600.
AF    Lib |The chart in [06286] has south on top.
AP    Lib |Z = 0.0486.
AQ    Lib |[Fe/H] = -0.60.
BE    Lib |The chart in [06286] is wrong.
BH    Lib |Recommended chart in [06286]: part III, page 50.
BT    Lib |Min II 12.3.
BW    Lib |The chart in [06286] is wrong.
CG    Lib |[Fe/H] = -1.82. P var. Max = 2438592.287 + 0.3068674d*E
CG    Lib |(JD2427800 - 39600) [07557]; since JD2439600 - see Table.
CQ    Lib |The coordinates in [01870] are wrong.
CZ    Lib |The chart in [06286], part I, page 40 is wrong. Recomended
CZ    Lib |chart in [06286]: part III, page 52.
EH    Lib |Delta(S) = 0. 9.35m <= Max < = 9.49m V;
EH    Lib |Max (A) = 2442162.556 + 0.273778d*E [09336].
ES    Lib |Min II 7.33.
EU    Lib |70d <= P <= 90d.
FI    Lib |90d <= P <= 110d.
FS    Lib |OH emission.
FX    Lib |Spectrum description  [06167,09371].
del   Lib |VB A (B 11.3m, 9", 351deg; C 12.80m, 67", 90deg); Min II
del   Lib |4.98. P var?
S     Lup |VB A (B = X Lup, 13", 176deg). P var. Max = 2411950 +
S     Lup |347.81d*E (JD2411950 - 14000); Max = 2414040 +
S     Lup |339.31d*E (JD2414000 - 19000); Max = 2419135 +
S     Lup |345.12d*E (JD2419000 - 26000); Max = 2426038 +
S     Lup |336.60d*E (JD2426000 - 29500); Max = 2429743 +
S     Lup |345.15d*E (JD2429500 - 35000); since JD2437600 - see Table.
X     Lup |VB B (A = S Lup).
Y     Lup |P var. Max = 2424691 + 408.15d*E (JD2423000 -
Y     Lup |25500); Max = 2425503 + 394.81d*E (JD2425500 -
Y     Lup |30250); Max = 2430641 + 407.75d*E (JD2430250 -
Y     Lup |35000); since JD2437900 - see Table.
RU    Lup |Sometimes varies quasiperiodically: P1 = 3.5457d, P2 =
RU    Lup |3.8375 [02412]. H2O maser.
RY    Lup |Quasiperiodicity: P = 3.7609d [09366].
SX    Lup |Min II 11.8.
TY    Lup |The chart in [06286] is wrong.
UX    Lup |[A/H] = -0.9. P var. P = 16.2403d (JD2411526 -
UX    Lup |14040); P = 16.2065d (JD2414040 - 24016); P =
UX    Lup |16.2492d (JD2424016 - 25638); P = 16.1794d
UX    Lup |(JD2425638 - 26449); P = 16.2241d (JD2426449 - 29693)
UX    Lup |[05387].
VV    Lup |Close northern companion.
VZ    Lup |P var? Light curve shape var?
CC    Lup |The chart in [06286] is wrong.
CW    Lup |The charts in [06286] are wrong.
CX    Lup |Min II 12.8.
CY    Lup |High Max every 360d, especially faint Min 80d before
CY    Lup |these high Max.
DG    Lup |Min II 15.1.
DQ    Lup |The chart in [06286] is wrong.
DY    Lup |In [00087] the information on variability of DY Lup is
DY    Lup |accompanied by the coordinates of DZ Lup and vice versa.
DY    Lup |The chart for DY Lup in [06286] is labeled DZ Lup, the
DY    Lup |chart for DZ Lup in [06286] is wrong.
DZ    Lup |In [00087] the information on variability of DY Lup is
DZ    Lup |accompanied by the coordinates of DZ Lup and vice versa.
DZ    Lup |The chart for DY Lup in [06286] is labeled DZ Lup, the
DZ    Lup |chart for DZ Lup in [06286] is wrong.
EL    Lup |VB.
ER    Lup |P2 = 140d.
EU    Lup |The chart in [06286] is wrong.
FK    Lup |Min II 10.7:.
FM    Lup |The chart in [02385] is wrong.
FR    Lup |Deep Min II.
FT    Lup |Min II 9.98. dI = 0.025P?, dII >= 0.066P. P var.
FT    Lup |Before JD2439300 Min I = 2427987.310 + 0.470089d*E
FT    Lup |[03948]; since JD2445000 - see Table. All the observations
FT    Lup |are well represented also by the elements:
FT    Lup |Min I = 2445061.834 + 0.470083d*E - 0.114d*10**(-9)*E**2
FT    Lup |[09360]. Light curve shape var?
FV    Lup |Min II 11.2.
GG    Lup |Min II 5.8.
GN    Lup |VB A (B 10.2m vis, 10", 98deg).
GO    Lup |Relatively short P.
GW    Lup |In the dark nebula Barnard 228.
HK    Lup |B - V: +1.23, +1.46.
HL    Lup |The initial identification with 2U 1543 - 47 is wrong.
HL    Lup |2U 1543 - 47 = IL Lup.
HM    Lup |B - V: +1.12.
HN    Lup |B - V: +1.55, +1.68.
HO    Lup |B - V: +0.70, +0.81.
alf   Lup |VB A (B 14.0m, 27.6", 232deg, 1901).
alf   Lup |Soft X-ray source. P2 = 3.145d is possible [08417].
gam   Lup |SB, Porb = 2.8081d.
del   Lup |Less probable variant of elements:
del   Lup |Max = 2441045.160 + 0.14273*E.
R     Lyn |S 4/5E - S 6/6 - .
S     Lyn |VB A (B 14m, 12.6", 155deg). P var. Max = 2414564 +
S     Lyn |300.26d*E (JD2414500 - 27400); Max = 2434241 +
S     Lyn |294.42d*E (JD2427400 - 35100); Max = 2440225 +
S     Lyn |300.44d*E (JD2435100 - 40220); since
S     Lyn |JD2440220 - see Table.
T     Lyn |P var. Max = 2425012 + 419.0d*E (JD2412800 - 34700);
T     Lyn |since JD2434700 - see Table.
U     Lyn |H2O, OH emission. P var. Max = 2417168 +
U     Lyn |440.3d*E (JD2417100 - 26000) [00458]; Max =
U     Lyn |2435908 + 432.05d*E (JD2426000 - 36000); Max =
U     Lyn |2439898 + 447.1d*E (JD2436000 - 40000); since
U     Lyn |JD2440000 - see Table.
V     Lyn |Cycles 55d and 87d replace one another. Mean brightness
V     Lyn |varies.
Y     Lyn |SB.
RR    Lyn |VB A (B 10m, 50"). Min II 5.90; Min II = 2438051.3115 +
RR    Lyn |9.945074d*E; E = 0.081; Min II - Min I = 0.45P (JD2437700).
RW    Lyn |[Fe/H] = -1.37.
RZ    Lyn |Min II 10.8.
SW    Lyn |Min II 9.65; dI = 0.038P. P var. Min I = 2425643.323 +
SW    Lyn |0.6440661d*E (JD2425640 - 35850) [02742]; Min I =
SW    Lyn |2438795.8016 + 0.6440520d*E (JD2438380 - 840)
SW    Lyn |[09387]; Min I = 2440614.0107 + 0.6440729d*E
SW    Lyn |(JD2439500 - 40620) [00001]; Min I = 2442786.4493 +
SW    Lyn |0.6440677d*E (JD2440650 - 42790) [07292];
SW    Lyn |since JD2442780 - see Table.
SX    Lyn |Min II 10.1. P var. Min I = 2428636.375 + 2.0225615d*E
SX    Lyn |(JD2427400 - 34700) [00519]; Min I = 2442561.424 +
SX    Lyn |2.0225172d*E (JD2442400 - 44000); since JD2444000 - see
SX    Lyn |Table.
SZ    Lyn |SB (Porb = 1146d, E = 0.26 [09388]). Delta(S) = 0.
SZ    Lyn |There is a periodical term in the elements:
SZ    Lyn |-0.00573d cos 2pi (EP0/P1 + 0.007); P0 = 0.120534920d,
SZ    Lyn |P1 = 1150d. Amplitude and shape of the light curve vary.
TT    Lyn |Delta(S) = 7.
TV    Lyn |[Fe/H] = -0.99.
TW    Lyn |Delta(S) = 10. P var. Max = 2418676.804 + 0.4817201d*E
TW    Lyn |(JD2418670 - 20155); Max = 2420155.685 + 0.4816929d*E
TW    Lyn |(JD2420155 - 27480); Max = 2427479.359 + 0.4817481d*E
TW    Lyn |(JD2427480 - 28630);
TW    Lyn |Max = 2428627.310 + 0.4818529d*E (JD2428620 - 37800)
TW    Lyn |[02819]. Since JD2445000 - see Table.
TZ    Lyn |Epoch of Min brightness is given.
UU    Lyn |Min II 11.82.
UV    Lyn |Min II 9.78.
UZ    Lyn |VR var (P = 0.065d [09392]).
VV    Lyn |VB A (B 11.76m, 38.6",354deg); SB; mu alpha = -0.0285S,
VV    Lyn |mu delta = -0.274".
VW    Lyn |P1 = 590s, P2 = 260s [09393].
CW    Lyn |Type RRC: is also possible.
S     Lyr |P var. Max = 2416186 + 432.01d*E (JD2415700 - 20100);
S     Lyr |Max = 2420961 + 445.83d*E (JD2420900 - 26500);
S     Lyr |Max = 2426748 + 429.01d*E (JD2426500 - 30700);
S     Lyr |Max = 2432357 + 441.88d*E (JD2432000 - 34600);
S     Lyr |since JD2442500 - see Table.
U     Lyr |VB A (B 13.0m, 9.4", 182deg). P var. Max = 2418345 +
U     Lyr |459.22d*E (JD2418000 - 27000); since JD2432000 - see
U     Lyr |Table.
V     Lyr |OH maser.
W     Lyr |P var. Max = 2415578 + 198.39d*E (JD2413000 - 19000);
W     Lyr |Max = 2420322 + 194.99d*E (JD2419000 - 25500);
W     Lyr |Max = 2431326 + 198.97d*E (JD2427000 - 31500);
W     Lyr |Max = 2432494 + 195.11d*E (JD2431500 - 36500);
W     Lyr |since JD2437500 - see Table.
Y     Lyr |Delta(S) = 0.8.
Z     Lyr |P var. Max = 2418150 + 285.07d*E (JD2417500 - 22200);
Z     Lyr |Max = 2423600 + 291.37d*E (JD2422200 - 29500);
Z     Lyr |Max = 2430000 + 284.00d*E (JD2429500 - 36800);
Z     Lyr |since JD2436800 - see Table.
RR    Lyr |mu alpha = -0.11", mu delta = -0.19". [Fe/H] = -1.14;
RR    Lyr |Delta(S) = 6. Blazhko effect of variable
RR    Lyr |amplitude (practically to complete disappearance of
RR    Lyr |Blazhko effect); Pi = 40.8d. Variations of Max light
RR    Lyr |phase up to 0.14P; magnitude in Max var in the range
RR    Lyr |up to 0.6m, that in Min var in the range up to 0.1m
RR    Lyr |[03418].According to [07270], a cycle ~4 yr is present
RR    Lyr |in Blazhko effect amplitude changes; at the end of
RR    Lyr |the cycle the Blazhko effect phase changes abruptly
RR    Lyr |by 0.25Pi. Magnetic field strength varies with the
RR    Lyr |pulsational period [09339].
RR    Lyr |P var. Max = 2414856.480 + 0.56682069d*E
RR    Lyr |(JD2414800 - 18800); Max = 2421854.052 + 0.56685169d*E
RR    Lyr |(JD2418800 - 26500) [09379]; Max = 2426571.3828 +
RR    Lyr |0.56684333d*E (JD2426500 - 32500) [09338]; Max =
RR    Lyr |2438215.9492 + 0.566830d*E (JD2438000 - 41000)
RR    Lyr |[05238]; Max = 2438215.9492 + 0.56683313d*E
RR    Lyr |(JD2441000 - 42900) [09338]; since JD2442900 - see Table.
RS    Lyr |P var. Max = 2415566 + 299.38d*E (JD2415000 - 24000);
RS    Lyr |Max = 2425176 + 308.08d*E (JD2424000 - 37200);
RS    Lyr |since JD2437200 - see Table.
RT    Lyr |P var. Max = 2437022 + 250.85d*E (JD2415000 - 39000);
RT    Lyr |since JD2439000 - see Table.
RU    Lyr |P var. Max = 2415983 + 370.70d*E (JD2415900 - 33000);
RU    Lyr |Max = 2433035 + 363.0d*E (JD2433000 - 41000);
RU    Lyr |since JD2441000 - see Table.
RV    Lyr |D = 0.015P. P var. Min = 2415949.7096 + 3.599007d*E
RV    Lyr |(JD2412185 - 16000); Min = 2415949.7096 +
RV    Lyr |3.599046d*E (JD2416000 - 21400) [00001];
RV    Lyr |Min = 2432015.671 + 3.5989845d*E (JD2421400 - 32000);
RV    Lyr |Min = 2432015.671 + 3.5990235d*E (JD2432000 -
RV    Lyr |39300) [09085]; since JD2442000 - see Table.
RW    Lyr |OH, H2O maser.
RX    Lyr |P var. Max = 2416226 + 249.94d*E (JD2415000 - 28800);
RX    Lyr |since JD2428800 - see Table.
RZ    Lyr |P var. Max = 2416415.360 + 0.51127069d*E
RZ    Lyr |(JD2413000 - 19000) [00001]; Max = 2426161.4375 +
RZ    Lyr |0.51124948D*E (JD2426000 - 38000) [00323];
RZ    Lyr |since JD2438000 - see Table.
RZ    Lyr |Blazhko effect, height of Max varies: 10.6m - 10.9m,
RZ    Lyr |Max (Delta(m)) = 2430904.3 + 116.654d*N + 0.01034d*N**2;
RZ    Lyr |Min (Delta(m)) - Max (Delta(m)) = 59.3d [03419].
RZ    Lyr |[Fe/H] = -1.69; Delta(S) = 10.0.
SS    Lyr |P var. Max = 2421695 + 350.48d*E (JD2416000 - 22500);
SS    Lyr |Max = 2429991 + 355.22d*E (JD2429000 - 38000); since
SS    Lyr |JD2438000 - see Table.
SZ    Lyr |According to [05750], during JD2434665 - 35044 the
SZ    Lyr |amplitude was twice smaller than usual (due to the depth
SZ    Lyr |of Min), and a temporary phase shift by 0.5P occured.
TT    Lyr |d = 0.010P; Min II 9.44.
TW    Lyr |VB A (B 15.2m pg, 14".70deg, 1912).
TY    Lyr |P var. Max = 2419285 + 336.49d:*E (JD2419000 - 23700);
TY    Lyr |Max = 2423985 + 329.79d*E (JD2423700 - 31250);
TY    Lyr |since JD2438600 - see Table.
TZ    Lyr |VB A (B 12.29m, 2.54", 2.5deg). Min II 11.05. P var.
TZ    Lyr |Min I = 2420669.480 + 0.5288234d*E (JD2420000 - 38000);
TZ    Lyr |since JD2438000 - see Table.
UX    Lyr |B - V: +0.11, +0.47.
UZ    Lyr |d = 0.012P:. P var. Min = 2424268.474 + 1.891253d*E
UZ    Lyr |(JD2422500 - 25500) [02087]; since JD2425500 - see Table.
AA    Lyr |Min II 13.5.
AH    Lyr |d = 0.03P. Min II 12.1.
AK    Lyr |Min II 12.9.
AL    Lyr |P var. Max = 2427865.82 + 12.9837d*E (JD2414800 - 28000)
AL    Lyr |[00001]; Max = 2432889.03 + 12.98047d*E
AL    Lyr |(JD2428000 - 35500) [04427]; since JD2435500 - see Table.
AQ    Lyr |P var. Max = 2425301.592 + 0.3571721d*E
AQ    Lyr |(JD2425300 - 29000); Max = 2428944.739 + 0.3571285d*E
AQ    Lyr |(JD2429000 - 30200); Max = 2430158.976 + 0.3571611d*E
AQ    Lyr |(JD2430200 - 33900); Max = 2433909.178 + 0.3571861d*E
AQ    Lyr |(JD2433900 - 35700); during JD2435700 - 37800 - see Table.
AQ    Lyr |Blazhko effect? According to visual observations,
AQ    Lyr |0.4m <= Delta(m) <= 1.2m.
AY    Lyr |Cycles of supermaxima 188.9d - 212.8d.
AY    Lyr |Superhumps period: Ps = 0.07552d [06249].
BF    Lyr |P var. Max = 2425296 + 130d*E (JD2425300 - 800);
BF    Lyr |During JD2429045 - 570 - see Table.
BH    Lyr |P var. Max = 2413712.358 + 0.6129028d*E
BH    Lyr |(JD2413712 - 27927); Max = 2434472.547 + 0.6128941d*E
BH    Lyr |(JD2434472 - 36102); since JD2436423 - see Table.
BQ    Lyr |Delta(S) = 0:.
BV    Lyr |d = 0.025P.
CC    Lyr |P var. Max = 2433182.7 + 24.028d*E (JD2426100 - 33400);
CC    Lyr |Max = 2437078.8 + 24.200d*E (JD2433400 - 37100) [00001];
CC    Lyr |Max = 2439418.5 + 24.185d*E (JD2437100 - 39420) [05644];
CC    Lyr |since JD2440400 - see Table. Light curve shape var?
CC    Lyr |[A/H] = -2.2.
CV    Lyr |Possible superposition of P2 = 135d.
CX    Lyr |P var. Max = 2418596.111 + 0.616689d*E
CX    Lyr |(JD2414880 - 20000); Max = 2427696.396 + 0.616669d*E
CX    Lyr |(JD2427530 - 30610); since JD2433000 - see Table.
CX    Lyr |Delta(S) = 7:.
DD    Lyr |P var. Max = 2425494.334 + 0.372610d*E (JD2418900 - 27600)
DD    Lyr |[00001]; since JD2427600 - see Table.
DF    Lyr |Min II 13.4.
DI    Lyr |P var. Max = 2437160.310 + 0.4174486d*E (JD2437160 - 39293);
DI    Lyr |Max = 2439293.468 + 0.4178451d*E (JD2439293 - 40768);
DI    Lyr |since JD2440768 - see Table.
DN    Lyr |P2 = 600d.
DR    Lyr |[Fe/H] =  -1.41; Delta(S) =7.4.
DU    Lyr |Min II 13.3.
EN    Lyr |B - V: + 0.40. + 0.43. P var. Delta(m) var.
EP    Lyr |Max I D = 0.20P; Min II 10.36m - 10.58m,  D = 0.50P;
EP    Lyr |Max II 10.01m - 10.10m,  D = 0.70P.
EP    Lyr |Secondary oscillations: P2 = 45.1d,  P3 = 7067d [09354].
EW    Lyr |P var; nonlinear term:
EW    Lyr |+0.00210d*10**(-6)*E**2 (JD2426500 - 45500);
EW    Lyr |since JD2442000 the observations are represented also by
EW    Lyr |the elements: Min = 2445597.391 + 1.948763d*E [07037,00001].
EX    Lyr |[Fe/H] = -0.63; Delta(S) = 2.5.
EZ    Lyr |VB A (B 12.3m, 14", 302deg, 1934). P var. Since
EZ    Lyr |JD2426577 - see Table. Delta(S) = 7.1.
FG    Lyr |VB A (B 14m, <10"). d = 0.035P. P var?
FH    Lyr |P var?
FK    Lyr |The identification with HDE 337663(G5) [00021] is wrong.
FL    Lyr |Min II 9.52,  DII = 0.05P.
FN    Lyr |B - V: +0.15, +0.48.
FO    Lyr |Min II 13.7.
GY    Lyr |The elements describe the brightest maxima. Between them
GY    Lyr |there are 2 - 3 waves of smaller amplitude. Red.
HP    Lyr |Min II 11.0.
HQ    Lyr |P var, periodic term: +30d*sin(8deg*E).
HT    Lyr |Min II 13.3.
HY    Lyr |Min II 14.1.
IK    Lyr |Blazhko effect?
IL    Lyr |According to [00569], Max = 2429375.519 + 0.377620d*E,
IL    Lyr |M - m = 0.14P:.
IO    Lyr |Delta(S) = 3.
IP    Lyr |Min II 13.3.
IW    Lyr |Min II 13.3.
IY    Lyr |Min II 14.1.
KM    Lyr |Blazhko effect: Pi = 30d, 0.14P <= M - m <= 0.20P.
KP    Lyr |ADS 11423 C (A 8.5m, B 9.7m; AB - C 77", 208deg; D 13.1m,
KP    Lyr |C - D 14", 61deg, 1904). P2 = 1300d is possible.
KR    Lyr |P var. The light curve shape var.
KT    Lyr |Min II 14.9.
KX    Lyr |Delta(S) = 0.
LQ    Lyr |[Fe/H] =  -1.39; Delta(S) = 7.2.
LR    Lyr |P var? [Fe/H] = -1.41; Delta(S) = 7.4.
LT    Lyr |Rapid variation (0.5m in an hour) were observed.
LX    Lyr |Delta(S) = 8:.
LZ    Lyr |P var. Min = 2425347.565 + 1.611143d*E (JD2425347 - 32119)
LZ    Lyr |[00569]; since JD2442870 - see Table.
MN    Lyr |Min II 14.1.
MR    Lyr |Alternative P = 0.66d:.
MS    Lyr |P < 0.5d?
MT    Lyr |Min II 16.2.
MV    Lyr |SB (Porb = 0.1336d [09373]).
MV    Lyr |Quasiperiodic fadings of different amplitude:
MV    Lyr |Min = 2425558 + 455.5d*E (JD2425500 - 30100);
MV    Lyr |Min = 2430113 + 325.3d*E (JD2430100 - 36900);
MV    Lyr |Min = 2436944 + 357.8d*E (JD2436900 - 44100) [09372].
MV    Lyr |After JD2444100 the mean brightness
MV    Lyr |level became fainter by 5m; outbursts with an amplitude
MV    Lyr |up to 3m of 1 - 2 months duration are observed [09404].
MV    Lyr |During the bright level of light, flickering up
MV    Lyr |to 0.4m in 5 Min in U bAnd is observed [00365]. Soft
MV    Lyr |X-ray source.
MV    Lyr |B - V: 0.00 +- 0.40; U - B:  -0.86 +  -1.30.
MW    Lyr |P var. Max = 2429521.386 + 0.3978817d*E (JD2427700 - 36000);
MW    Lyr |since JD2436000 - see Table.
MW    Lyr |Blazhko effect: Pi = 33.3d; the amplitude varies by 0.6m.
MZ    Lyr |Min II 14.0.
NV    Lyr |d = 0.02P:.
NW    Lyr |P var. Max = 2436483.323 + 1.6012330d*E (JD2414500 -
NW    Lyr |36400) [03506]; since JD2436400 - see Table.
NW    Lyr |B - V: +0.38, +0.86.
NY    Lyr |Min II 13.1.
NZ    Lyr |O - C vary harmonically with an amplitude +- 0.01d,
NZ    Lyr |Pi ~2500P.
OQ    Lyr |VB (B 12.1m vis, 5.3", 175deg, 1930).
OS    Lyr |40d <= P <= 60d. P2 = 400d - 500d is superimposed.
PQ    Lyr |d = 0.014P; Min II 14.9.
PS    Lyr |d = 0.02P:; Min II 11.4.
PU    Lyr |Close companions sf, s.
PV    Lyr |d = 0.03P:.
PY    Lyr |Min II 13.4. P var. Min I = 2434980.4372 + 0.38576671d*E
PY    Lyr |(JD2432700 - 36900) [04248]; since JD2442500 - see Table.
QQ    Lyr |Min II 14.6.
QT    Lyr |Min II 14.6.
QU    Lyr |Min II 13.1.
V0335 Lyr |Large scatter in the light curve.
V0336 Lyr |P var. Min = 2429965.283 + 1.9049105d*E (JD2429370 - 31590);
V0336 Lyr |during JD2438930 - 40010 - see Table.
V0337 Lyr |Large scatter in the light curve.
V0348 Lyr |Min II 16.8.
V0348 Lyr |The elements are valid during JD2444023 - 45232.
V0350 Lyr |P var. The elements are valid during JD2438280 - 45232.
V0355 Lyr |The elements are valid during JD2429322 - 45232.
V0356 Lyr |VB A (B 17.5m, 10", 120deg, [00001]).
V0361 Lyr |Min II 15.3, Max II 14.7, Max II - Min I = 0.70P.
V0361 Lyr |The elements are valid during JD2433776 - 45232).
V0374 Lyr |Faint companions np, sf.
V0380 Lyr |Faint close companion nf.
V0385 Lyr |Faint close companion sf.
V0388 Lyr |No brightenings were observed during JD2438322 - 39289.
V0389 Lyr |The elements are valid during JD2438322 - 40007.
V0390 Lyr |The elements are valid during JD2439913 - 40007.
V0401 Lyr |Min II 14.4:. The period may be spurious.
V0403 Lyr |P var?, Pi = 500 P?
V0404 Lyr |Min II 12.4.
V0406 Lyr |Min II 13.0.
V0409 Lyr |P var? The elements are valid during JD2434500 - 40000.
V0409 Lyr |Blazhko effect?
V0411 Lyr |Min II 14.4. Alternatively RRC (P = 0.291315d).
V0412 Lyr |Min II 14.1; Min II - Min I = 0.48P.
V0413 Lyr |Min II 14.8?
V0415 Lyr |Cycle <= 150d.
V0417 Lyr |Min II 16.2. P var?
V0418 Lyr |P var. The elements are valid during JD2437100 - 40400.
V0423 Lyr |Min II 15.5. P var?
V0424 Lyr |Blazhko effect?
V0428 Lyr |Min II 14.3. Apsidal motion?
V0429 Lyr |Min II 14.8?
V0431 Lyr |Min II 15.1.
V0435 Lyr |Possibly ew with twice longer P. P may be spurious.
V0462 Lyr |P var? The elements are valid during JD2439913 - 40007.
V0467 Lyr |Min II 12.9. JD2415288 - 43287; the elements
V0467 Lyr |are valid during JD2415288 - 43287; large scatter
V0467 Lyr |on the light curve. According to [09412], during
V0467 Lyr |JD2443424 - 44165 the light variation range is 12.4m -
V0467 Lyr |12.6m pg, the elements are not valid.
V0470 Lyr |U = 0.40", p = 7deg. P1 = 738.6s, P2 = 557.4s, P3 = 318.0s,
V0470 Lyr |P4 = 291.9s, P5 = 259.1s.
V0473 Lyr |P var, Delta(m) var. According to [09413], P =
V0473 Lyr |1.490795d + 1.22d*10**(-6)*(JD - 2443600)/365.25d.
V0473 Lyr |Cyclic P variations: P alpha = 1178.5d; Pt = 2655d.
V0473 Lyr |Delta(m) varies with the period P alpha; P4 = 1063.5d
V0473 Lyr |may be traced in the variations of Vr.
V0473 Lyr |0.06m <= Delta(m) <= 0.36m.
V0474 Lyr |P2 = 76d.
V0477 Lyr |The central star of planetary nebula Abell 46. Strong
V0477 Lyr |reflection effect. Depths of minima: Min I 1.42m B,
V0477 Lyr |Min II ~0.1m B.
V0531 Lyr |Minima observed only between JD 2448600 and 2448800.
V0550 Lyr |SB, Porb = 1.0309d.
alf   Lyr |IR excess.
bet   Lyr |ADS 11745 A (B 8.6m, B7V, 46", 149deg; C 13.0m, 47",
bet   Lyr |248deg). Min II 3.85. P var. Nonlinear terms:
bet   Lyr |+3.883d*10**(-6)*E**2 - 0.10d*10**(-10)*E**3.
bet   Lyr |Light curve shape var.
bet   Lyr |Radio and X-ray source. IR excess.
del 2 Lyr |Open cluster delta**2 Lyr member [02505].
R     Men |Sometimes P = 120d;
R     Men |Sometimes P = 240d.
T     Men |In the Large Magellanic Cloud region; not a member of the
T     Men |Cloud. There is a sguare term in the elements:
T     Men |+8.1d*10**(-6)*E**2.
U     Men |VB A (B 10.4m, 0.6", 71deg, 1935.3). A var
U     Men |(0.8m <= A <= 2.9M). P var. Max = 2416927 + 426.9d*E
U     Men |(JD2415200 - 17400) [00207]; since JD2417400 - see Table.
V     Men |Epoch corresponds to the middle of
V     Men |the light curve ascending branch.
W     Men |The member of the Large Magellanic Cloud.
RR    Men |Min II 12.1.
RS    Men |In the Large Magellanic Cloud region; not
RS    Men |a member of the Cloud.
RT    Men |In the Large Magellanic Cloud region; not a member of
RT    Men |the Cloud.
RU    Men |In the Large Magellanic Cloud region; not a member of
RU    Men |the Cloud.
RV    Men |In the Large Magellanic Cloud region; not a member of
RV    Men |the Cloud.
RW    Men |In the Large Magellanic Cloud region; not a member of
RW    Men |the Cloud.
TU    Men |Porb = 0.1176d [09376]. Superhump
TU    Men |Period Ps = 0.12625d [04772].
TY    Men |Min II 8.47; d I = 0.00P, d II = 0.07P.
TY    Men |Shape of the light curve varies.
TZ    Men |Min II 6.36.
UX    Men |Min II 9.47; Min II - Min I = 0.50045P.
UX    Men |One of the components may be a physical variable.
WY    Men |In the region of the NGC 1841 globular cluster; not a
WY    Men |member of the cluster. In the halo of the magellanic
WY    Men |clouds system.
WZ    Men |In the region of the NGC 1841 globular cluster, not a
WZ    Men |member of the cluster. In the halo of the Magellanic
WZ    Men |Clouds system.
XX    Men |In the region of the NGC 1841 globular cluster, not a
XX    Men |member of the cluster. In the halo of the Magellanic
XX    Men |Clouds system.
XY    Men |In the Large Magellanic Cloud region; not a member of the
XY    Men |Cloud. Min II 10.88; dI = 0.05P; dII = 0.00P.
XZ    Men |There are there oscillations simultaneously: P1 = 0.1083d
XZ    Men |(A1 = 0.0094m B), P2 = 0.0855d (A2 = 0.0082m B),
XZ    Men |P3 = 0.0955d (A3 = 0.0058m B); P2/P1 = 0.789.
AN    Men |Type RRC: is also possible.
iot   Men |Min II 6.05.
R     Mic |P var. Max = 2413373 + 138.60d*E (JD2413300 - 29600)
R     Mic |[00458]; Max = 2432745 + 137.43d*E (JD2429600 - 34700);
R     Mic |Max = 2435091 + 140.84d*E (JD2434700 - 37800);
R     Mic |since JD2437800 - see Table.
S     Mic |P var. Max = 2413499 + 214.5d*E (JD2413500 - 15900) [00458];
S     Mic |Max = 2432102 + 208.23d*E (JD2422700 - 32200);
S     Mic |since JD2432200 - see Table.
U     Mic |OH, H2O emission.
V     Mic |OH, H20 emission.
Y     Mic |Mean brightness varies.
Z     Mic |(k - b)2 = 0.12; Delta(S) = 4.
RR    Mic |[A/H] = -1.4. P var. Max = 2433032.96 + 31.78175d*E
RR    Mic |(JD2415000 - 35300) [02747]; since JD2443600 - see Table.
RY    Mic |P var? Elements given in the Table represent observations
RY    Mic |in the interval JD2436100 - 40210.
RY    Mic |According to [00085] Max = 2428670 + 190d*E.
RZ    Mic |Min II 11.2.
TV    Mic |Min II 12.4.
UZ    Mic |Min II 12.4.
VW    Mic |In the interval JD2436600 - 840)
VW    Mic |Max = 2436807.248 + 0.35620d*E. Since JD2442600 - see
VW    Mic |Table.
WY    Mic |P = 0.511427d? [00001].
XZ    Mic |In the interval JD2436670 - 840 Max =
XZ    Mic |2436731.480 + 0.449208d*E. Since JD2442630 - see Table.
ZZ    Mic |(k - b)2 = 021; Delta(S) = 0. P var? Max = 2437192.3131 +
ZZ    Mic |0.0671786d*E (JD2437180 - 460) [04308];
ZZ    Mic |Max = 2439320.2162 + 0.0671575d*E (JD2439320 - 340)
ZZ    Mic |[05683]; since JD2440440 - see Table.
ZZ    Mic |Further period increase is possible [09380]. According
ZZ    Mic |to [07985] there are two simultaneous oscillations with the
ZZ    Mic |periods P1 and P2: P1 = 0.0654d, P2 = 0.0513d.
ZZ    Mic |P2/P1 = 0.784; A2(U) = 0.25 A1(U).
AE    Mic |In the interval JD2436670 - 840 Max =
AE    Mic |2436728.470 + 0.324142d*E. Since JD2442630 - see Table.
AH    Mic |Min II 13.6.
AT    Mic |VB (A 10.83m V, M 4.5Ve; B 10.9m V, M 4.5Ve; a =
AT    Mic |6.40", P = 675 yr, e = 0.60 [09381].
AT    Mic |mu alpha = + 0.0216s, mu delta = -0.331" (mu, Vr,
AT    Mic |pi - common with AU Mic).
AT    Mic |Unusually high freguency of flares
AT    Mic |allows to suppose that both components are variable.
AT    Mic |The range of combined brightness variation of the
AT    Mic |system is given in the Table.
AU    Mic |mu alpha = +0.0212S, mu delta = -0.348" (mu, pi,
AU    Mic |Vr - common with AT Mic). SB? 0.20P <= M - m <= 0.55P.
AU    Mic |There are periodical light variations and also flares with
AU    Mic |A <= 0.5m U [08601].
AW    Mic |mu alpha = +0.0077s, mu delta = -0.089".
AW    Mic |Shape of the light curve strongly varies. Multiperiodicity
AW    Mic |is possible.
AX    Mic |mu alpha = -0.2805s, mu delta = -1.152". In
AX    Mic |minimum brightness B - V = +1.42, U - B = +1.20.
R     Mon |Peculiar non-stellar object at the apex of the reflection
R     Mon |variable [09396] cometary nebula NGC 2261. Probably young
R     Mon |star surrounded by dust cloud. Light curve in [09394].
S     Mon |In the open star cluster
S     Mon |NGC 2264. VB A (B 8.2m, 2.9", 213deg; 9.9m, 16.6", 14deg.)
T     Mon |SB (Porb> = 70 yr [09397]). [A/H] = 0.3.
T     Mon |There is a sguare term in the elements given in the
T     Mon |Table: +5.34d*10**(-6)*E**2.
T     Mon |Deviations from the parabola in the O - C, E diagram
T     Mon |have a wave-like trend. If this wave is attributed to
T     Mon |the light-time effect, Porb = 100 years.
T     Mon |The observations are also satisfied by the following
T     Mon |system of linear elements: Max = 2412874.56 + 27.0093d*E
T     Mon |(JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E
T     Mon |(JD2415250 - 27150); since JD2427150 -
T     Mon |Max = 2436137.090 + 27.0205d*E [02392].
U     Mon |P var. Min = 2408897 + 92.26d*E (JD2408800 - 36210) [00368];
U     Mon |since JD2437300 - see Table.
U     Mon |Mean magnitude varies with the period 2320d [00657].
U     Mon |Spectrum investigation [02226].
V     Mon |P var. Max = 2412172 + 334.5d*E (JD2412000 - 23500) [00458];
V     Mon |Max = 2427870 + 332.5d*E (JD2423500 - 28200);
V     Mon |Max = 2429904 + 342.0d*E (JD2428200 - 30800);
V     Mon |Max = 2439570 + 331.6d*E (JD2430800 - 41225);
V     Mon |since JD2441225 - see Table.
X     Mon |P var. Max = 2415078 + 154.0d*E (JD2415000 - 18800);
X     Mon |Max = 2419758 + 149.6d*E (JD2419700 - 21000);
X     Mon |Max = 2421136 + 155.0d*E (JD2421000 - 24600);
X     Mon |Max = 2424673 + 169d*E (JD2424600 - 25600);
X     Mon |Max = 2425644 + 155.6d*E (JD2425600 - 26800);
X     Mon |Max = 2427028 + 150.7d*E (JD2427000 - 28000) [00458];
X     Mon |Max = 2429521 + 155.8d*E (JD2428000 - 36300);
X     Mon |Max = 2438846 + 145.3d*E (JD2437800 - 38900); since
X     Mon |JD2440800 - see Table. The amplitude strongly varies;
X     Mon |sometimes irregular light variations are observed.
Y     Mon |P var. Max = 2415792 + 228.6d*E (JD2415300 - 19700);
Y     Mon |Max = 2419928 + 227.4d*E (JD2419700 - 24300) [00458];
Y     Mon |Max = 2432647 + 233.3d*E (JD2424300 - 32900);
Y     Mon |since JD2432900 - see Table.
RR    Mon |P var. Max = 2417476 + 384.5d*E (JD2417400 - 19600) [00458];
RR    Mon |since JD2419600 - see Table.
RU    Mon |Min II 11.06; D II var: 0.06P <= DII <= 0.12P;
RU    Mon |Min II - Min I var: 0.25P < = Min II - Min I <= 0.75P.
RU    Mon |P var. In the interval JD2429100 - 38409 Min I =
RU    Mon |2418357.0140; 3.5846794d(E - 406) - 0.429d cos alpha +
RU    Mon |0.06d*sin(2alpha) + 0.010d*cos(3alpha) +
RU    Mon |0.003d*sin(4alpha), MinII = 2418355.2220 +
RU    Mon |3.5846794d(E - 406) + 0.429d cos alpha +
RU    Mon |0.060D*sin(2alpha) - 0.010d cos*3alpha +
RU    Mon |0.003d*sin(4alpha) (JD2416900 - 29100);
RU    Mon |Min I = 2429641.567 + 3.5846391d*(E - 3554) -
RU    Mon |0.429d*cos(alpha) + 0.060d*sin(2alpha) + 0.010d*cos(3alpha) +
RU    Mon |0.003d*sin(4alpha),
RU    Mon |Min II = 2429639.775 + 3.5846391d(E - 3554) +
RU    Mon |0.429d*cos(alpha) + 0.060d*sin(2alpha) -
RU    Mon |0.010d*cos(3alpha) + 0.003d*sin(4alpha), where alpha =
RU    Mon |0.01245deg(E - 406) [03445].
RU    Mon |The epochs E are being calculated for Min I from JD hel.
RU    Mon |2416901.205, and for Min II - from JD hel. 2416900.248.
RU    Mon |In the interval JD2438409 - 41743
RU    Mon |Min I = 2438409.6045 + 3.584586d(E - 6000) -
RU    Mon |0.4290d*cos(alpha) + 0.0620d*sin(2alpha) +
RU    Mon |0.0107d*cos(3alpha) + 0.0026d*sin(4alpha) -
RU    Mon |0.00036d cos 5alpha, Min II = 2438407.8122 +
RU    Mon |3.584586d(E - 6000) + 0.4290d cos alpha +
RU    Mon |0.0620d*sin(2alpha) - 0.0107d*cos(3alpha) +
RU    Mon |0.0026d*sin(4alpha) + 0.00036d*cos(5alpha),
RU    Mon |where alpha = 0.012385deg(E - 406) [07987].
RU    Mon |since JD2441743 - Min I = 2441743.2633 +
RU    Mon |3.584670d(E - 6930) - 0.4336d cos alpha +
RU    Mon |0.0634d*sin(2alpha) + 0.0111d*cos(3alpha) +
RU    Mon |0.0021d*sin(4alpha), Min II = 2441741.4710 +
RU    Mon |3.584689d(E - 6930) + 0.4336d cos alpha +
RU    Mon |0.0634d*sin(2alpha) - 0.0111d*cos(3alpha) +
RU    Mon |0.0021d*sin(4alpha), where alpha = 70.6deg +
RU    Mon |0.0114deg(E - 6094) [09546]. Linear elements for Min I
RU    Mon |epochs in 1973 - 1990 are given in the Table.
RU    Mon |Corresponding elements for Min II epochs are:
RU    Mon |Min II = 2441741.575 + 3.584567d*E. E = 0.38.
RU    Mon |Apsidal motion period is 285 years.
RV    Mon |Mean brightness varies with P = 1047d.
RW    Mon |Min II 9.45; d I = 0.027P, d II = 0.023P. P var.
RW    Mon |Min I = 2417943.687 + 1.9061012d*E (JD2417940 - 32900)
RW    Mon |[03450]; since JD2432900 - see Table.
RX    Mon |P var. Max = 2418980 + 343.2d*E (JD2416200 -
RX    Mon |19000); Max = 2423097 + 338.9d*E (JD2422000 -
RX    Mon |28500); since JD2428500 - see Table.
RY    Mon |VB A (B 12.29M, 28").
SS    Mon |In the region of the open cluster NGC 2264.
SU    Mon |S 5/7 - S 6/7. P var: 69d (JD2416700 - 19100); 203.5d
SU    Mon |(JD2420100 - 22920); 69d (JD2423000 - 30100).
SU    Mon |In the intervals JD2423000 - 520 - const (11.5m),
SU    Mon |JD2424820 - 980 - const (11.8m).
SV    Mon |[A/H] = 0.2. P var. Max = 2419041.805 + 15.230721d*E
SV    Mon |(JD2412000 - 22000) [00025]; Max = 2422651.931 +
SV    Mon |15.23256d*E (JD2422600 - 23850) [09400]; Max =
SV    Mon |2424571.60 + 15.2513d*E (JD2423850 - 24600);
SV    Mon |Max = 2434045.326 + 15.2304d*E (JD2424600 - 34100);
SV    Mon |since JD2433000 - see Table.
SX    Mon |Mean brightness varies with P = 1100d.
SZ    Mon |VB A (B 11m - 12m, 10" [09401]). Min II 10.55. P var.
SZ    Mon |Min I = 2426357.1 + 32.760d*E (JD2422000 - 26400);
SZ    Mon |Min I = 2427861.2 + 32.708d*E (JD2426750 - 32000);
SZ    Mon |since JD2432800 - see Table.
SZ    Mon |Shape of the light curve varies. Heights of maxima and
SZ    Mon |depths of minima are constant.
TU    Mon |Min II 9.1.
TV    Mon |In the region of the open star cluster NGC 2237.
TW    Mon |Wachmann [03453] assigns the variable to the RRab
TW    Mon |type with the elements Max = 2433001.371 + 0.8743887*E,
TW    Mon |but notes a considerable dispersion of the points around
TW    Mon |the mean light curve obtained with this period. As the
TW    Mon |periods by Hessner (PH) and Wachmann (PW) are mutually
TW    Mon |related (1/PW ~1/PH + 1) it is more probable on account of
TW    Mon |the above mentioned circumstance that the variable belongs
TW    Mon |to cepheids.
TX    Mon |[A/H] = -0.3.
UV    Mon |The form of the light curve being unusual for RR Lyr type
UV    Mon |variables (Max II 13.5 at the phase 0.39P, Min II 13.8
UV    Mon |at the phase 0.22P), the period may be doubtful,
UV    Mon |though it was found independently by two investigators
UV    Mon |[00380,03453].
UX    Mon |Min II 8.52; dI = 0.044P. P var?
UX    Mon |Brightness in maximum varies with the amplitude up to 0.2m.
VV    Mon |Min II 9.55; dI = dII = 0.07P.
VV    Mon |There is a square term in the elements given in the Table:
VV    Mon |-0.12d*10**(-7)*E**2.
VW    Mon |P var. Max = 2425243.40 + 0.6041350d*E (JD2414700 -
VW    Mon |30700); since JD2430700 - see Table.
VW    Mon |In [00386,05448] And other previous works the spurious
VW    Mon |period value 1.532d is being accepted suggesting the
VW    Mon |curious nature of the variable. Serious observations are
VW    Mon |necessary to select the true value of the period.
VX    Mon |Depth of Min II 0.07m.
VY    Mon |In the region of the nebula IC 446.
XX    Mon |[A/H] = -0.2.
XZ    Mon |Min II 13.6; d = 0.02P:.
AA    Mon |[A/H] = -0.9. P var. Max = 2430788.266 + 3.938052d*E
AA    Mon |(JD2425300 - 34800) [03453]; since JD2434800 - see Table.
AC    Mon |In the region of the open cluster NGC 2323.
AK    Mon |P var. Max = 2425279 + 319.2d*E (JD2425200 - 28000); since
AK    Mon |JD2428000 - see Table.
AN    Mon |Min II 11.7:; d = 0.027P.
AO    Mon |Min II 10.16; DII = 0.14P; Min II - Min I = 0.4933P. P var.
AO    Mon |Min I = 2426735.333 + 1.884758d*E (JD2426700 - 40000);
AO    Mon |since JD2440000 - see Table.
AQ    Mon |Min II 10.9; DII = 0.05P; dI = 0.014P.
AR    Mon |Min II 9.03; d = 0.011P.
AR    Mon |There is a square term in the elements given in the Table:
AR    Mon |-1.22d*10**(-6)*E**2.
AU    Mon |Min II 8.2:. Shape of the light curve varies.
AU    Mon |Brightness in maximum varies periodically with the
AU    Mon |amplitude 0.2m: Max = 2443105 + 411d*E; M - m = 0.5P.
AV    Mon |Depth of Min II 0.04m.
AW    Mon |P var. Min = 2425649.053 + 20.797d*E (JD2425500 -
AW    Mon |26400) [09408]; Min = 2426439.340 + 20.81905d*E
AW    Mon |(JD2426400 - 35900) [00511]; since JD2435900 - see Table.
AX    Mon |Binary system with an envelope and gaseous streams.
AX    Mon |Porb = 232.60d [06103]. Spectrum investigation [09411].
AX    Mon |Epoch of Min brightness preceeding the moment of
AX    Mon |conjunction for 0.25p is given in the Table; A = 0.4m U.
AX    Mon |Besides periodical variations, there are rapid light
AX    Mon |fluctuations up to 0.1m.
BB    Mon |Depth of Min II 0.04m.
BC    Mon |P var. Max = 2421240 + 275.8d*E (JD2421200 -
BC    Mon |25960); Max = 2428880 + 267.2d*E (JD2425960 -
BC    Mon |30000); since JD2430000 - see Table.
BE    Mon |Delta(S) = 0.
BH    Mon |d = 0.01p:.
BM    Mon |Min II 12.3. According to [09415], apsidal motion is
BM    Mon |possible.
BO    Mon |Min II 10.1. P var. Min I = 2428211.596 + 2.2251753d*E
BO    Mon |(JD2415000 - 36000) [00007]; since JD2436000 - see Table.
BP    Mon |P var?
BP    Mon |Elements given in the Table are valid in the interval
BP    Mon |JD2425600 - 29700.
BT    Mon |VB A (B 16.0m, 10", 0deg).
BT    Mon |After the outburst in 1939 the brightness varies in the
BT    Mon |range 16.0m - 18.7m with the elements: Min =
BT    Mon |2443491.7155 + 0.3338141d*E; D = 0.20p, 0 <= d < = 0.03p.
BT    Mon |Before the outburst in 1939, according to [09417],
BT    Mon |the following elements were valid: Min = 2429500.207 +
BT    Mon |0.3338010d*E. Emission nebula with the radius of 3.8"
BT    Mon |was discovered in 1981 around the nova [09148].
BX    Mon |Usually was considered as mira type variable
BX    Mon |[09421]. In the Table the epoch of light maximum and
BX    Mon |the period are given according to [09419]. According
BX    Mon |to [09420] the Balmer emission lines originate in the
BX    Mon |nebulosity surrounding the symbiotic system and are
BX    Mon |excited by the hot component, and light variations
BX    Mon |are due to the orbital motion in the system.
BZ    Mon |d = 0.030P. In the region of the open cluster CR 106.
CC    Mon |In the region of the open cluster CR 106.
CD    Mon |P var. Max = 2427704 + 273.8d*E (JD2427400 - 30400); since
CD    Mon |JD2430400 - see Table.
CE    Mon |Min II 14.2.
CF    Mon |Min II 13.7; d = 0.02P:.
CH    Mon |d = 0.030P.
CS    Mon |VB A (B 13m, 9", 0deg).
CT    Mon |In the region of the open cluster NGC 2244.
CU    Mon |[A/H] = -0.2.
CV    Mon |In the centre of an anonymous open cluster.
CV    Mon |VB A (B 13.76m, 10", 270deg; C 13.72m, 14", 270deg).
CV    Mon |P var. Max = 2429805.142 + 5.378782d*E (JD2429360 -
CV    Mon |36000); since JD2436000 - see Table.
DD    Mon |Min II 11.3.
DF    Mon |The chart in [05285] is wrong, the star observed was
DF    Mon |not DF Mon.
DN    Mon |Min II 13.9.
DR    Mon |In the region of the open cluster Cr 106.
DT    Mon |P var. Max = 2425324 + 345d*E (JD2425300 - 28200)
DT    Mon |In the interval JD2429250 - 37700 there were cycles 119d,
DT    Mon |230d, 350d.
DW    Mon |In the region of the open cluster NGC 2286.
EE    Mon |P var. Max = 2425300.42 + 4.80776d*E (JD2425300 -
EE    Mon |27720); since JD2427720 - see Table.
EH    Mon |d = 0.023P.
EK    Mon |P var. Max = 2425302.59 + 3.95773d*E (JD2425200 -
EK    Mon |33000) [00387]; since JD2433000 - see Table.
EP    Mon |d = 0.026P.
ES    Mon |d = 0.02P.
EW    Mon |Min II 14.2.
FH    Mon |Depth of Min II 0.04m.
FP    Mon |In the region of the open cluster NGC 2353.
FS    Mon |Min II 11.2.
FU    Mon |S 6.5/7.5.
FW    Mon |d = 0.016P. Depth of Min II 0.04m.
FX    Mon |OH emission.
FZ    Mon |The elements should be checked.
GH    Mon |Min II 13.1.
GP    Mon |In the region of the open cluster NGC 2264.
GQ    Mon |In the region of the open cluster NGC 2264.
GR    Mon |In the region of the open cluster NGC 2264.
GU    Mon |Min II 12.5.
GV    Mon |Depth of Min II 0.04m.
GX    Mon |OH, H2O, SIO maser.
HI    Mon |Min II 9.9.
HM    Mon |Min II 13.6. P var. Min I = 2430110.1948 + 0.40765737d*E
HM    Mon |(JD2429600 - 35400) [05285]; since JD2435400 - see Table.
HO    Mon |d = 0.03P.
HP    Mon |d = 0.04P:.
HR    Mon |Depth of Min II 0.03m.
HY    Mon |Min II 12.4.
IL    Mon |d = 0.03P.
IM    Mon |Min II 6.47.
IO    Mon |In the region of the open cluster NGC 2264.
IP    Mon |In the region of the open cluster NGC 2264.
IQ    Mon |In the region of the open cluster NGC 2264.
IR    Mon |P var?
IS    Mon |Depth of Min II 0.05m.
IX    Mon |Min II 12.8.
IZ    Mon |Min II 12.0.
KU    Mon |In the region of the open cluster NGC 2264.
KV    Mon |In the region of the open cluster NGC 2264.
KW    Mon |In the region of the open cluster NGC 2264.
KX    Mon |In the region of the open cluster NGC 2264.
KY    Mon |In the region of the open cluster NGC 2264.
KZ    Mon |In the region of the open cluster NGC 2264.
LL    Mon |In the region of the open cluster NGC 2264.
LM    Mon |In the region of the open cluster NGC 2264.
LN    Mon |In the region of the open cluster NGC 2264.
LO    Mon |In the region of the open cluster NGC 2264.
LP    Mon |In the region of the open cluster NGC 2264.
LQ    Mon |In the region of the open cluster NGC 2264.
LR    Mon |In the region of the open cluster NGC 2264.
LS    Mon |In the region of the open cluster NGC 2264.
LT    Mon |In the region of the open cluster NGC 2264.
LU    Mon |In the region of the open cluster NGC 2264.
LV    Mon |In the region of the open cluster NGC 2264.
LW    Mon |In the region of the open cluster NGC 2264.
LX    Mon |In the region of the open cluster NGC 2264.
LY    Mon |In the region of the open cluster NGC 2264.
LZ    Mon |In the region of the open cluster NGC 2264.
MM    Mon |In the region of the open cluster NGC 2264.
MN    Mon |In the region of the open cluster NGC 2264.
MO    Mon |VB A (B 20m, 10", 356deg); in the region of the
MO    Mon |open cluster NGC 2264.
MP    Mon |In the region of the open cluster NGC 2264.
MQ    Mon |In the region of the open cluster NGC 2264.
MX    Mon |Min II 11.7.
NN    Mon |Min II 12.9.
NS    Mon |Min II 11.1.
NT    Mon |In the region of the open cluster NGC 2264.
NU    Mon |In the region of the open cluster NGC 2264.
NV    Mon |In the region of the open cluster NGC 2264.
NW    Mon |In the region of the open cluster NGC 2264.
NX    Mon |In the region of the open cluster NGC 2264.
NY    Mon |In the region of the open cluster NGC 2264.
NZ    Mon |In the region of the open cluster NGC 2264.
OO    Mon |In the region of the open cluster NGC 2264.
OP    Mon |In the region of the open cluster NGC 2264.
OQ    Mon |In the region of the open cluster NGC 2264.
OR    Mon |In the region of the open cluster NGC 2264.
OS    Mon |In the region of the open cluster NGC 2264.
OT    Mon |In the region of the open cluster NGC 2264.
OU    Mon |In the region of the open cluster NGC 2264.
OV    Mon |In the region of the open cluster NGC 2264.
OW    Mon |In the region of the open cluster NGC 2264.
OX    Mon |VB A (B 15m, 7", 35deg); in the region of the open
OX    Mon |cluster NGC 2264.
OY    Mon |In the region of the open cluster NGC 2264.
OZ    Mon |In the region of the open cluster NGC 2264.
PP    Mon |In the region of the open cluster NGC 2264.
PQ    Mon |In the region of the open cluster NGC 2264.
PR    Mon |The elements should be checked.
PT    Mon |In the region of the open cluster NGC 2264.
PU    Mon |In the region of the open cluster NGC 2264.
PV    Mon |In the region of the open cluster NGC 2264.
PW    Mon |In the region of the open cluster NGC 2264.
PX    Mon |In the region of the open cluster NGC 2264.
PY    Mon |In the region of the open cluster NGC 2264.
QR    Mon |290d <= P <= 400d. Depth of Min varies by
QR    Mon |0.9m with the period about 2000d.
QT    Mon |In the region of the open cluster NGC 2264.
QU    Mon |In the region of the open cluster NGC 2264.
QV    Mon |In the region of the open cluster NGC 2264.
QW    Mon |In the region of the open cluster NGC 2264.
QX    Mon |In the region of the open cluster NGC 2264.
QY    Mon |In the region of the open cluster NGC 2264.
QZ    Mon |In the region of the open cluster NGC 2264.
V0334 Mon |In the region of the open cluster NGC 2264.
V0335 Mon |In the region of the open cluster NGC 2264.
V0336 Mon |In the region of the open cluster NGC 2264.
V0337 Mon |In the region of the open cluster NGC 2264.
V0338 Mon |In the region of the open cluster NGC 2264.
V0339 Mon |In the region of the open cluster NGC 2264.
V0340 Mon |In the region of the open cluster NGC 2264.
V0341 Mon |In the region of the open cluster NGC 2264.
V0342 Mon |In the region of the open cluster NGC 2264.
V0343 Mon |In the region of the open cluster NGC 2264.
V0344 Mon |In the region of the open cluster NGC 2264.
V0345 Mon |In the region of the open cluster NGC 2264.
V0346 Mon |In the region of the open cluster NGC 2264.
V0347 Mon |VB A (B 20m, 12", 120deg); in the region of the open
V0347 Mon |cluster NGC 2264.
V0348 Mon |In the region of the open cluster NGC 2264.
V0349 Mon |In the region of the open cluster NGC 2264.
V0350 Mon |In the region of the open cluster NGC 2264.
V0351 Mon |In the region of the open cluster NGC 2264.
V0352 Mon |In the region of the open cluster NGC 2264.
V0353 Mon |In the region of the open cluster NGC 2264.
V0354 Mon |In the region of the open cluster NGC 2264.
V0355 Mon |In the region of the open cluster NGC 2264.
V0356 Mon |VB (3", 78deg); in the region of the open cluster
V0356 Mon |NGC 2264.
V0357 Mon |In the region of the open cluster NGC 2264.
V0358 Mon |In the region of the open cluster NGC 2264.
V0359 Mon |In the region of the open cluster NGC 2264.
V0360 Mon |In the region of the open cluster NGC 2264.
V0361 Mon |In the region of the open cluster NGC 2264.
V0362 Mon |In the region of the open cluster NGC 2264.
V0363 Mon |In the region of the open cluster NGC 2264.
V0364 Mon |In the region of the open cluster NGC 2264.
V0365 Mon |VB B (A = V591 Mon, B 7", 135deg); in the region of the
V0365 Mon |open cluster NGC 2264.
V0366 Mon |In the region of the open cluster NGC 2264.
V0367 Mon |In the region of the open cluster NGC 2264.
V0368 Mon |VB (9", 252deg); in the region of the open cluster
V0368 Mon |NGC 2264.
V0369 Mon |VB (11", 264deg); in the region of the open cluster
V0369 Mon |NGC 2264.
V0370 Mon |VB (8", 97deg); in the region of the open cluster
V0370 Mon |NGC 2264.
V0371 Mon |In the region of the open cluster NGC 2264.
V0372 Mon |SC 7/7.5.
V0373 Mon |In the region of the open cluster NGC 2264.
V0379 Mon |d = 0.015P:.
V0380 Mon |Min II 12.9; P = 1.98904166d?
V0383 Mon |Min II 15.2.
V0384 Mon |Min II 13.0.
V0389 Mon |Min II 14.9.
V0393 Mon |Min II 14.3.
V0394 Mon |d = 0.02P; depth of Min II 0.04m.
V0395 Mon |d = 0.03P.
V0396 Mon |Min II 13.5.
V0397 Mon |Min II 11.9.
V0398 Mon |In the region of the open cluster NGC 2264.
V0399 Mon |In the region of the open cluster NGC 2264.
V0400 Mon |In the region of the open cluster NGC 2264.
V0401 Mon |In the region of the open cluster NGC 2264.
V0402 Mon |In the region of the open cluster NGC 2264.
V0403 Mon |In the region of the open cluster NGC 2264.
V0404 Mon |d = 0.02P:.
V0405 Mon |In the region of the open cluster NGC 2264.
V0406 Mon |In the region of the open cluster NGC 2264.
V0407 Mon |In the region of the open cluster NGC 2264.
V0408 Mon |In the region of the open cluster NGC 2264.
V0409 Mon |In the region of the open cluster NGC 2264.
V0410 Mon |In the region of the open cluster NGC 2264.
V0411 Mon |In the region of the open cluster NGC 2264.
V0412 Mon |In the region of the open cluster NGC 2264.
V0413 Mon |In the region of the open cluster NGC 2264.
V0414 Mon |In the region of the open cluster NGC 2264.
V0415 Mon |In the region of the open cluster NGC 2264.
V0416 Mon |In the region of the open cluster NGC 2264.
V0417 Mon |In the region of the open cluster NGC 2264.
V0418 Mon |In the region of the open cluster NGC 2264.
V0419 Mon |In the region of the open cluster NGC 2264.
V0420 Mon |In the region of the open cluster NGC 2264.
V0421 Mon |In the region of the open cluster NGC 2264.
V0422 Mon |In the region of the open cluster NGC 2264.
V0423 Mon |In the region of the open cluster NGC 2264.
V0424 Mon |In the region of the open cluster NGC 2264.
V0425 Mon |In the region of the open cluster NGC 2264.
V0426 Mon |VB A (B = NSV 3125 17.0m, 6", 117deg); in the region of
V0426 Mon |the open cluster NGC 2264.
V0427 Mon |In the region of the open cluster NGC 2264.
V0428 Mon |In the region of the open cluster NGC 2264.
V0429 Mon |In the region of the open cluster NGC 2264.
V0430 Mon |In the region of the open cluster NGC 2264.
V0431 Mon |In the region of the open cluster NGC 2264.
V0432 Mon |In the region of the open cluster NGC 2264.
V0433 Mon |In the region of the open cluster NGC 2264.
V0434 Mon |In the region of the open cluster NGC 2264.
V0435 Mon |In the region of the open cluster NGC 2264.
V0436 Mon |In the region of the open cluster NGC 2264.
V0437 Mon |In the region of the open cluster NGC 2264.
V0438 Mon |In the region of the open cluster NGC 2264.
V0439 Mon |In the region of the open cluster NGC 2264.
V0440 Mon |In the region of the open cluster NGC 2264.
V0441 Mon |In the region of the open cluster NGC 2264.
V0442 Mon |Min II 11.6.
V0443 Mon |In the region of the open cluster NGC 2264.
V0444 Mon |In the region of the open cluster NGC 2264.
V0445 Mon |Min II 11.3.
V0446 Mon |[A/H] = -0.7.
V0447 Mon |[A/H] = -1.4.
V0448 Mon |Min II 9.8.
V0449 Mon |d = 0.02P.
V0450 Mon |Min II 12.6.
V0451 Mon |Min II 14.7.
V0452 Mon |Min II 12.7; d = 0.02P.
V0453 Mon |Min II 11.8.
V0454 Mon |Min II 12.2.
V0455 Mon |Min II 15.3.
V0456 Mon |Min II 13.7.
V0457 Mon |Min II 14.3; d = 0.03P:.
V0458 Mon |Min II 13.8.
V0459 Mon |Min II 14.7.
V0460 Mon |Min II 10.7.
V0463 Mon |d = 0.03P; P = 2.2476768d?
V0464 Mon |Min II 12.3.
V0465 Mon |P var. Max = 2429642.44 + 2.71341d*E (JD2425600 -
V0465 Mon |30800) [03551]; Max = 2431845.65 + 2.713212d*E
V0465 Mon |(JD2430000 - 35200) [03453]; Max = 2435541.315 +
V0465 Mon |2.713668d*E (JD2435200 - 41600); since JD2441600 - see
V0465 Mon |Table.
V0466 Mon |VB A (B 15m, 135deg).
V0474 Mon |(k - b)2 = 0.32. Blazhko effect:
V0474 Mon |Max(O - C) = 2441664.962 + 7.74639d*N; Min(O - C) =
V0474 Mon |2441669.569 + 7.74639d*N; 0.03m <= A <= 0.37m;
V0474 Mon |-0.02d <= O - C <= +0.03d. Freguency analysis gives
V0474 Mon |three principal oscillations [08669]: P1 = 0.1361258d
V0474 Mon |(A1 = 0.18m), P2 = 0.1337745d (A2 = 0.12m),
V0474 Mon |P3 = 0.1385591d (A3 = 0.04m).
V0478 Mon |In the region of the nebula IC 2169.
V0479 Mon |In the region of the nebula IC 2169.
V0481 Mon |In the region of the nebula IC 2169.
V0482 Mon |In the region of the nebula IC 2169.
V0483 Mon |In the region of the nebula IC 2169.
V0486 Mon |VB A (B 18.4M, 6"). In the region of the nebula NGC 2245.
V0487 Mon |In the region of the nebula NGC 2245.
V0488 Mon |In the region of the nebula NGC 2245.
V0489 Mon |In the region of the nebula NGC 2245.
V0490 Mon |In the region of the nebula NGC 2247.
V0493 Mon |In the region of the open cluster Tr 5.
V0494 Mon |Depth of Min II 0.05m.
V0496 Mon |Min II 12.8.
V0497 Mon |8.9 - 11.8 IR.
V0498 Mon |P = 2.4727818d?
V0500 Mon |In the region of the open cluster NGC 2264.
V0501 Mon |Min II 13.1; Min II - Min I = 0.445P; DII = 0.036P.
V0503 Mon |9.2 - 10.9 IR.
V0505 Mon |Min II 7.55.
V0507 Mon |SB2 (P = 53.781d [09483]); d = 0.015P:.
V0510 Mon |[A/H] = -0.1.
V0513 Mon |Depth of Min II 0.04m.
V0514 Mon |Min II 13.3.
V0515 Mon |Min II 12.7.
V0521 Mon |Min II 10.4.
V0524 Mon |Min II 15.2.
V0526 Mon |P var. Max = 2433304.284 + 2.675208d*E (JD2429300 -
V0526 Mon |35170); since JD2439170 - see Table.
V0527 Mon |Depth of Min II 0.05m.
V0530 Mon |Min II 12.8.
V0532 Mon |Min II 12.8. RRC?
V0535 Mon |P var. Max = 2431846.445 + 0.3328791d*E
V0535 Mon |(JD2429600 - 34060); since JD2434060 - see Table.
V0535 Mon |[Fe/H] = -1.44.
V0539 Mon |In the region of the open cluster NGC 2244.
V0540 Mon |In the region of the nebula IC 446.
V0541 Mon |In the region of the nebula IC 446.
V0542 Mon |In the region of the nebula IC 446.
V0543 Mon |In the region of the open cluster NGC 2244.
V0544 Mon |In the region of the open cluster NGC 2244.
V0545 Mon |In the region of the open cluster NGC 2244.
V0546 Mon |In the region of the open cluster NGC 2244.
V0547 Mon |In the region of the open cluster NGC 2244.
V0548 Mon |In the region of the open cluster NGC 2244.
V0549 Mon |In the region of the open cluster NGC 2244.
V0550 Mon |VB A (B 17.3m, 6", 0deg ); in the region of the open
V0550 Mon |cluster NGC 2244.
V0551 Mon |In the region of the open cluster NGC 2244.
V0552 Mon |In the region of the open cluster NGC 2244.
V0553 Mon |In the region of the open cluster NGC 2244.
V0554 Mon |In the region of the open cluster NGC 2244.
V0555 Mon |In the region of the open cluster NGC 2244.
V0556 Mon |In the region of the open cluster NGC 2244.
V0557 Mon |In the region of the open cluster NGC 2244.
V0560 Mon |Depth of Min II 0.05m.
V0565 Mon |Connected with the diffuse nebula
V0565 Mon |NGC 2313 having diameter of 10" and a faint cometary
V0565 Mon |nebula.
V0569 Mon |VB A (B 10.8m, 6.2", 281deg; C 10.5m, 38.3", 295deg).
V0569 Mon |The range of combined light variation of A and B
V0569 Mon |components is given. According to [08215], P = 0.18d.
V0571 Mon |(k - b)2 = 0.32.
V0571 Mon |Non-radial pulsation with variable periods:
V0571 Mon |P1 = 0.0999081d (A1 = 0.052m), P2 = 0.0749998d
V0571 Mon |(A2 = 0.015m) (JD2440914 - 41692) [07127]; P1 = 0.0894534d
V0571 Mon |(A1 = 0.038m), P2 = 0.15988d (A2 = 0.025m), P3 = 0.106516d
V0571 Mon |(A3 = 0.014m). P4 = 0.26998d (A4 = 0.012m), P5 = 0.15069d
V0571 Mon |(A5 = 0.011m) (JD2441662 - 719) [09450].
V0577 Mon |VB (A 11.3m V, B 14.8m V; a = 0.312", P = 16.60 yr, e =
V0577 Mon |0.38); mu alpha = +0.049S, mu beta = +0.73".
V0577 Mon |Both components are probably variables. The range
V0577 Mon |of combined light variation of the system is given
V0577 Mon |in the Table [06146].
V0578 Mon |In the region of the open cluster NGC 2244.
V0579 Mon |In the region of the open cluster NGC 2264.
V0580 Mon |In the region of the open cluster NGC 2264.
V0581 Mon |In the region of the open cluster NGC 2264.
V0582 Mon |In the region of the open cluster NGC 2264.
V0583 Mon |In the region of the open cluster NGC 2264.
V0584 Mon |In the region of the open cluster NGC 2264.
V0585 Mon |In the region of the open cluster NGC 2264.
V0586 Mon |In the region of the open cluster NGC 2264.
V0588 Mon |In the region of the open cluster NGC 2264.
V0589 Mon |In the region of the open cluster NGC 2264.
V0590 Mon |VB (10", 358deg); in the region of the open cluster
V0590 Mon |NGC 2264.
V0591 Mon |VB A (B = V365 Mon, 7", 135deg); in the region of the open
V0591 Mon |cluster NGC 2264.
V0593 Mon |In the region of the open cluster NGC 2264.
V0594 Mon |In the region of the open cluster NGC 2264.
V0595 Mon |In the region of the open cluster NGC 2264.
V0596 Mon |In the region of the open cluster NGC 2264.
V0597 Mon |In the region of the open cluster NGC 2264.
V0598 Mon |In the region of the open cluster NGC 2264.
V0599 Mon |In the region of the open cluster NGC 2264.
V0600 Mon |In the region of the open cluster NGC 2264.
V0601 Mon |In the region of the open cluster NGC 2264.
V0602 Mon |In the region of the open cluster NGC 2264.
V0603 Mon |In the region of the open cluster NGC 2264.
V0604 Mon |In the region of the open cluster NGC 2264.
V0605 Mon |In the region of the open cluster NGC 2264.
V0606 Mon |In the region of the open cluster NGC 2264.
V0607 Mon |In the region of the open cluster NGC 2264.
V0608 Mon |In the region of the open cluster NGC 2264.
V0609 Mon |In the region of the open cluster NGC 2264.
V0610 Mon |In the region of the open cluster NGC 2264.
V0611 Mon |In the region of the open cluster NGC 2264.
V0612 Mon |In the region of the open cluster NGC 2264.
V0613 Mon |S 3/2.
V0616 Mon |Novalike outbursts were observed in 1917 (Max JD2421540)
V0616 Mon |and in 1975 (Max JD2442646). In quiescent state probably
V0616 Mon |ellipsoidal light variation is observed with P = 0.325d
V0616 Mon |and A = 0.2m [09458], and also slower light variations
V0616 Mon |with P = 7.39d [09459] or 7.8d [09460]. Spectrum description
V0616 Mon |[09461,09462].
V0624 Mon |In the region of the open cluster Cr 106.
V0628 Mon |In the region of the open cluster NGC 2264.
V0629 Mon |In the region of the open cluster NGC 2264.
V0630 Mon |VB A (B 21m, 3", 300deg); in the region of the open
V0630 Mon |cluster NGC 2264.
V0632 Mon |In the region of the open cluster NGC 2368.
V0637 Mon |Basic oscillation with A1 = 0.05m and elements given in
V0637 Mon |the Table is superimposed by the second one with
V0637 Mon |A2 = 0.02m and the elements: Max = 2443496.1624 +
V0637 Mon |0.19740d*E. Beat period Pb = 6.09d.
V0638 Mon |VB (6.5m, 8.5m; 0.8", 178deg).
V0640 Mon |In the region of the open cluster NGC 2244.
V0640 Mon |Porb = 14.39604d [06103].
V0640 Mon |Irregular light variations.
V0640 Mon |Probably transitional stage from a binary system of
V0640 Mon |O stars to a system of WR type [04107].
V0641 Mon |VB A (B 10.91m, 21.4", 310deg; C 12.46m, 25.8", 285deg).
V0641 Mon |In the region of the open cluster NGC 2264.
V0642 Mon |In the region of the open cluster NGC 2264. Cluster
V0642 Mon |non-member. Epoch of light minimum is
V0642 Mon |given in the Table.
V0645 Mon |Epoch of light minimum is given in the Table.
V0741 Mon |Type ACV: is also possible.
V0750 Mon |In the region of the nebula IC 2177.
V0753 Mon |Type ACV: is also possible.
S     Mus |Marked on the chart for BO Mus. Max II = Max I,
S     Mus |D (Max II) = 0.15P. P var? SB 1 (Porb = 506.4d).
T     Mus |P2 = 1021d.
V     Mus |In the Coal Sack region.
RV    Mus |P = 128d: is possible.
RW    Mus |P = 130d: is possible.
RY    Mus |V1 (NGC 4833).
RZ    Mus |V2 (NGC 4833). Cluster non-member.
SY    Mus |Min II 11.2; Min I - Min II = 170d.
SY    Mus |Elements for Min I of quasiperiodic variations observed
SY    Mus |during JD2434910 - 41510 are given. Radio source.
TU    Mus |Min II 8.65. P var. Min I = 2424260.396 + 1.38728d*E
TU    Mus |(JD2423900 - 29300) [00039]; during JD2437380 - 41900 - see
TU    Mus |Table. The light curve shape var.
TV    Mus |Min II 11.3.
TW    Mus |Min II 12.4.
TZ    Mus |B - V: +1.22, +1.43.
UW    Mus |Min II 11.9.
UY    Mus |Min II 12.0.
VW    Mus |Min II 13.9.
WY    Mus |P var. Periodic term: +0.35d*sin(0.12deg*E).
XZ    Mus |Before JD2419200 Max = 2412590 + 113d*E.
AB    Mus |Min II 13.0.
AS    Mus |[A/H] = 0.5.
AX    Mus |P var. During JD2412550 - 19200 - see Table; during
AX    Mus |JD2423900 - 26100 P = 97.3d.
AY    Mus |Min II 10.8. Min II - Min I = 0.481P.
AY    Mus |The elements are valid during 1897 - 1943. In the time
AY    Mus |interval JD2441683 - 721 eclipses did not occur [08094].
BB    Mus |P, possibly P should be doubled.
BD    Mus |Depth of Min II 0.05m.
BE    Mus |Min II 14.1.
BF    Mus |Min II 14.4.
BK    Mus |P very long P: 56d < d < 310d.
BR    Mus |Min II 11.25. B - V: +0.10m.
BS    Mus |Min II 11.5.
BX    Mus |Depth of Min II 0.04m.
CD    Mus |Min II 14.7.
CS    Mus |P > 120d.
DW    Mus |According to [08135], the spectral type is M5e, typical of
DW    Mus |Mira stars. Elements in [03934] were deduced from the
DW    Mus |observed brightness variations with P ~355d which
DW    Mus |was considered to be a spurious period; rapid variations
DW    Mus |were confirmed by 7h of photographic observations.
DZ    Mus |Possibly Pshould be doubled.
EE    Mus |In the coal sack. The flare was observed spectroscopically.
EN    Mus |d = 0.035P:.
EP    Mus |[A/H] = 0.2. According to [08136], EA,
EP    Mus |P = 4.15d, D = 0.05P, 11.63m - 12.60m V, Min II 11.7:.
ET    Mus |Alternatively possible type EW [08727,04001].
EV    Mus |d = 0.09P:.
EY    Mus |In the Coal Sack region.
EZ    Mus |Alternative possible values of P 4.3032d, 4.3224d.
FH    Mus |Depth of Min II 0.03m.
FO    Mus |P var?
GK    Mus |Min II 15.0.
GN    Mus |Min II 14.2.
GO    Mus |Min II 15.2.
GP    Mus |B - V: +1.03, +1.61.
KU    Mus |Type RV: is also possible.
alf   Mus |VB A (B 13.0m, 29.3", 316deg).
eta   Mus |VB A (B 7.30m, 60").
tet   Mus |VB (A 5.64m, B 7.5m, 5.3", 187deg); SB (Porb = 18.341B).
tet   Mus |Variable intensity of emission lines with respect to the
tet   Mus |continuum (double wave; elements in the Table are for the
tet   Mus |epochs of Min I variability in the UV range (lambda lambda
tet   Mus |1550 - 3300 A) with an amplitude about 2%, P = 1.5d and
tet   Mus |rapid changes (lamda lamda 1550 - 1800 A) with an
tet   Mus |amplitude about 3 - 5% on the time scale of 50s - 70s
tet   Mus |[08532]. Connected with a nebula, 80'*45'.
R     Nor |VB A (B 14.0m, 5.7", 268deg, 1929). P var. Max II =
R     Nor |2406371 + 486.94d*E (JD2406300 - 25000); Max II =
R     Nor |2426359 + 500.56d*E (JD2426000 - 30500); Max II =
R     Nor |2431377 + 489.0d*E (JD2430500 - 34500); since
R     Nor |JD2437600 - see Table. Like R Cen, has a doudle Max,
R     Nor |JD2437600 - see Table. Like R Cen, has a doudle Max,
R     Nor |divided by a comparatively shallow Min II. Max II is
R     Nor |usually brighter than Max I. D (Min I) = 0.43P,
R     Nor |D (Max I) = 0.70P, D(Min II) = 0.85P.
S     Nor |In the centre of the open cluster NGC 6087, cluster member.
S     Nor |[A/H] = -0.1.
T     Nor |P var.Max = 2414783 + 241.87d*E (JD2414700 - 28000);
T     Nor |Max = 2428084 + 244.93d*E (JD2428000 - 35000);
T     Nor |since JD2437000 - see Table.
U     Nor |P var. Max = 2415028.94 + 12.64084d*E (JD2415000 - 26000)
U     Nor |[00060]; since JD2434000 - see Table, [A/H] = -0.6.
W     Nor |P2 ~1300d.
Y     Nor |VB A (B 12.2m vis, 4.0", 156deg, 1903).
Z     Nor |Min II 9.6.
RR    Nor |Min II 9.9.
RS    Nor |B - V: +1.13,  +1.48.
RT    Nor |Quasiperiodic variations: P1 ~59d, P2 ~175d [08140].
RV    Nor |[A/H] = 0.8.
RV    Nor |There are irregularities in the light curve.
SV    Nor |Min II 12.6.
SW    Nor |d = 0.003P.
SX    Nor |d = 0.1P.
SY    Nor |VB A (B 12.8m, 2.1", 315deg, 1934). B - V: +1.16,  +1.49.
SY    Nor |[A/H] = 0.5.
SZ    Nor |Min II 12.6.
TT    Nor |Twice longer P is possible.
TU    Nor |Min II 12.5. Associated with a small faint nebula.
TV    Nor |Min II 9.3.
TW    Nor |In the region of the poor open cluster Lynga 6.
TW    Nor |B - V: +1.79, +2.22. [A/H] = 0.2.
TX    Nor |Min II 12.5.
TZ    Nor |Min II 12.1.
UV    Nor |d ~0.07P.
UX    Nor |In Max light B - V = +0.30.
UY    Nor |d = 0.025P.
UZ    Nor |d = 0.02P.
VV    Nor |In the region of the cluster NGC 6152.
VX    Nor |Depth of Min II ~0.03m.
VZ    Nor |In the region of the cluster NGC 6152. Min II 14.3.
WX    Nor |The chart is erroneously labelled as that for WZ Nor.
WX    Nor |Min II 12.8.
WZ    Nor |The chart is erroneously labelled as that for WX Nor.
WZ    Nor |Min II 13.4.
XY    Nor |Min II 13.2.
AA    Nor |[A/H] = -0.1.
AF    Nor |In the region of the open cluster NGC 5999.
AQ    Nor |The chart in [06286] is wrong.
AR    Nor |The chart in [06286] is wrong.
AT    Nor |d = 0.026P:.
BE    Nor |Min II 14.2.
BF    Nor |The chart in [06286] is wrong.
BH    Nor |Min II 13.2.
BP    Nor |Close companion.
CE    Nor |d = 0.05P. Min II 11.8?
CG    Nor |The chart in [06286] is wrong.
CI    Nor |The chart in [06286] is wrong.
CT    Nor |The chart in [06286] is wrong.
CX    Nor |Min II 15.0.
DE    Nor |The chart in [06286] is wrong.
DF    Nor |The chart in [06286] is wrong.
DO    Nor |Min II 14.2. In the region of the open cluster NGC 6087.
DP    Nor |The chart in [06286] is wrong.
DR    Nor |In the region of the open cluster NGC 6087.
EE    Nor |The chart in [06286] is wrong.
EM    Nor |Min II 13.8.
ET    Nor |d = 0.032P.
FG    Nor |The chart in [06286] is wrong.
FI    Nor |The chart in [06286] is wrong.
FK    Nor |Min II 15.0.
FQ    Nor |According to [00060], P = 1.994d?
FW    Nor |Min II 14.5.
GM    Nor |d = 0.02P; Min II 11.01; Min II - Min I = 0.499P
GM    Nor |(JD2441683 - 721), Min II - Min I = 0.531P (JD2425381 -
GM    Nor |28402). B - V = 0.44m.
GN    Nor |Min II 13.3, DII = 0.16P, Min II - Min I = 0.405P
GN    Nor |(JD2425900). Apsidal motion: P = 500yr.
GO    Nor |Min II 13.7.
GQ    Nor |Min II 13.8.
GR    Nor |[A/H] = 0.9.
GT    Nor |d = 0.048P.
GU    Nor |In the region of the open cluster NGC 6067.
GU    Nor |B - V: +1.17, +1.40. [A/H] = 0.1.
GV    Nor |d = 0.03P:.
GX    Nor |Min II 15.0.
HH    Nor |VB B (A 9.9m vis, FO; B 12.6", 148deg). d = 0.05P.
HI    Nor |D is very small.
HK    Nor |Min II 12.9.
HO    Nor |Min II 13.2:.
HW    Nor |d = 0.024P.
HZ    Nor |P = 2.921584d is possible.
IQ    Nor |B - V: +1.55, +1.93.
IS    Nor |In the region of the open cluster NGC 6067.
IT    Nor |Min II 9.8.
KL    Nor |P >= 140d.
KM    Nor |P >= 170d.
KQ    Nor |Mira Ceti type is not excluded [04001].
KT    Nor |P >= 180d.
KX    Nor |Min II 14.8.
LO    Nor |P >= 220d.
LV    Nor |Deep Min II.
LX    Nor |Possible P values: 0.60492d, 0.7851d, etc.
NR    Nor |Min II 15.9.
NW    Nor |P > 140d.
NX    Nor |Min II 14.4.
OS    Nor |Epoch of Min is given. EW/KW type is possible.
OT    Nor |Min II 13.7.
OU    Nor |Min II 15.1.
OV    Nor |P >= 200d.
OW    Nor |P >= 120d.
OX    Nor |P >= 110d.
PQ    Nor |Possibly a cepheid which is a fainter component of an
PQ    Nor |unresolved binary. Epoch of Max is given.
PT    Nor |In the region of the open cluster NGC 6067.
QT    Nor |HV 5388 = HV 8903. The coordinates in [00424] are wrong.
QV    Nor |3U 1538 - 52. No.12 [04124].
QV    Nor |Epoch of Min corresponding to the X-ray eclipse is given.
QV    Nor |Depth of Min I 0.05m V, that of Min II 0.08m V. The period
QV    Nor |of X-ray pulses Px = 528.928s [04114]. A flare was observed
QV    Nor |with Delta(m) > 0.3m [09456].
QX    Nor |4U 1608 - 52.
QZ    Nor |In the open cluster NGC 6067.
V0367 Nor |May be not a supergiant.
V0374 Nor |Type LBV: is also possible.
mu    Nor |In the region of the open cluster NGC 6169.
U     Oct |P var. Max = 2420685 + 302.00d*E (JD2414900 -
U     Oct |20700); Max = 2424320 + 300.74d*E (JD2422800 -
U     Oct |29800); Max = 2431901 + 309.60d*E (JD2429800 -
U     Oct |32250); Max = 2434018 + 300.70d*E (JD2432250 -
U     Oct |38800); since JD2438800 - see Table.
X     Oct |P var.Max = 2415170 + 208.40d*E (JD2415100 -
X     Oct |17100); Max = 2417425 + 201.24d*E (JD2417100 -
X     Oct |20700); Max = 2423780 + 207.95d*E (JD2422000 -
X     Oct |24000); Max = 2424370 + 200.18d*E (JD2424000 -
X     Oct |25600); since JD2425600 - see Table. Depths of minima are
X     Oct |stongly variable; 1.1m <= A <= 4.0m.
RV    Oct |Delta(S) = 10.
TX    Oct |Min II 12.7.
UV    Oct |Delta(S) = 9; (k - b)2 = 0.06. Blazhko effect: P = 80d;
UV    Oct |0.14P <= M - m <= 0.24P, 0.4m <= A <= 1.3m.
UZ    Oct |Min II 9.48; dI = 0.00P, dII = 0.05P. P var. Min I =
UZ    Oct |2440223.1560 + 1.1493709d*E (JD2438300 - 42000);
UZ    Oct |since JD2442000 - see Table.
AM    Oct |Min II 14.9.
BE    Oct |P < 20d:.
BG    Oct |P = 0.7490d?
BK    Oct |Min II 14.6.
BP    Oct |(k - b)2 = 0.25.
CC    Oct |Basic radial pulsation with P1 = 0.12490d (A1 = 0.042m)
CC    Oct |is superimposed by others with periods: P2 = 0.0795317d
CC    Oct |(A2 = 0.008m), P3 = 0.12336d (A3 = 0.014m); P4 =
CC    Oct |0.11068d (A4 = 0.008m), P5 = 0.12713d (A5 = 0.006m);
CC    Oct |P6 = 0.11815d (A6 = 0.006m).
CD    Oct |mu = 0.51", p = 279deg. One of the periods P = 686s
CD    Oct |(A = 0.01m).
CE    Oct |Light oscillation with P2 = 0.054511d (A2 = 0.0056m) is
CE    Oct |superimposed by an oscillation with P1 = 0.2100d or
CE    Oct |0.2660d (A1 = 0.0052m), which is due to pulsation or
CE    Oct |ellipsoidal variability in a close binary system.
CP    Oct |Variability type and spectral type (F2/F3Ib/II) do not agree.
alf   Oct |SB, Porb = 9.073d.
R     Oph |P var. Max = 2399214 + 302.1d*E (JD2399200 - 2427900)
R     Oph |[00458]; Max = 2427915 + 304.0d*E (JD2427900 - 34900);
R     Oph |Max = 2434906 + 301.5d*E (JD2434900 - 40600) [00001];
R     Oph |since JD2440600 - see Table.
U     Oph |ADS 10428 A (B 12.26m, GOV, 20.4", 358deg). Min II 6.46.
U     Oph |P var. Periodic term:
U     Oph |+0.0120d*sin(0.0483deg*E + 4.7833deg).
V     Oph |P var. Max = 2411155 + 296.73d*E (JD2411000 - 24000);
V     Oph |Max = 2424198 + 302.46d*E (JD2424000 - 28000);
V     Oph |since JD2428000 - see Table.
W     Oph |P var. Before JD2420500 Max = 2415186 +
W     Oph |335.07d*E; Max = 2420870 + 325.33d*E (JD2420500 -
W     Oph |24700); since JD2424700 - see Table.
X     Oph |VBA (A = 0.34", Porb = 485.3 yr; B - 9m, K1III, 0.4",
X     Oph |142deg, 1980).
X     Oph |The range of the combined brightness is given.
X     Oph |P var. Max = 2416416 + 336.61d*E (JD2416400 - 26000);
X     Oph |Max = 2426161 + 331.28d*E (JD2426000 - 32500); Max =
X     Oph |2432788 + 335.50d*E (JD2432500 - 38000);
X     Oph |since JD2438000 - see Table.
Y     Oph |SB1? Porb = 2612d? P var. Before JD2427000
Y     Oph |Max = 2408694.77 + 17.11884d*E; since
Y     Oph |JD2432000 - see Table. [A/H] = -0.2.
Z     Oph |P var. Max = 2411896 + 349.0d*E (JD2411800 - 21000)
Z     Oph |[00458]; Max = 2420962 + 352.1d*E (JD2421000 - 25000);
Z     Oph |Max = 2425183 + 347.4d*E (JD2425000 - 31000);
Z     Oph |Mean elements after JD2431000 - see Table.
RR    Oph |P var. Nonlinear term: -0.009282d*E2.
RS    Oph |Previous outbursts: 1898, 1933, 1958.
RS    Oph |According to [07575], in 1972 - 1973 there were semiregular
RS    Oph |variations (Delta(m) ~0.5M, P = 50D - 70D).
RT    Oph |P var. Before JD2426500 Max = 2417452 +
RT    Oph |429.00d*E; Max = 2426461 + 422.67d*E (JD2426500 -
RT    Oph |34000); since JD2434500 - see Table. OH, H2O maser.
RU    Oph |P var. Before JD2422000 Max = 2417388 +
RU    Oph |200.95d*E; Max = 2422011 + 203.62d*E (JD2422000 -
RU    Oph |27300); Max = 2427298 + 200.5d*E (JD2427300 - 29000);
RU    Oph |Max = 2429305 + 203.88d*E (JD2429000 - 33000);
RU    Oph |during JD2433000 - 40500 - see Table.
RV    Oph |d = 0.015P; Min II 9.56, DII = 0.09P. The light curve
RV    Oph |share var.
RW    Oph |P var. Max = 242494 + 247.86d*E (JD2425000 - 34000).
RW    Oph |The Table gives mean elements.
RX    Oph |OH, H2O maser.
RY    Oph |P var. Max = 2415235 + 151.05d*E (JD2414700 - 24000);
RY    Oph |Max = 2424152 + 149.69d*E (JD2424000 - 31000); Max =
RY    Oph |2431339 + 150.94d*E (JD2431000 - 40000);
RY    Oph |since JD2440000 - see Table.
RZ    Oph |d = 0.030P.
SS    Oph |P var. Before JD2432500 Max = 2417330 + 179.88d*E.
ST    Oph |(k - b)2 = 0.03.
SV    Oph |The elements are valid since JD2422000.
SW    Oph |VB A (B 12.0m vis, 2.4", 91deg, 1943). d = 0.02P. P var.
SW    Oph |Min = 2418880.528 + 2.445948d*E (JD2418880 - 26200)
SW    Oph |[00001]; Min = 2431235.216 + 2.446086d*E (JD2427900 -
SW    Oph |33500) [02389]; since JD2434000 - see Table.
SX    Oph |d = 0.03P.
SZ    Oph |P var. Before JD2428400 Min = 2421057.556 + 3.708454d*E;
SZ    Oph |since JD2442000 - see Table.
TT    Oph |[Fe/H] = -0.5.
TW    Oph |P2 = 2000d:. Associated with a nebula of variable
TW    Oph |brightness [03479].
UU    Oph |d = 0.024P. P var?
UX    Oph |P var. Max = 2426041 + 117.34d (JD2406430 - 28040);
UX    Oph |since JD2433100 - see Table.
VW    Oph |P var. Mean elements are given. During JD2422500 - 30600
VW    Oph |Max = 2430554 + 282.69d*E.
WW    Oph |Epoch of Min is given. The chart in [06286] is wrong.
WZ    Oph |Min II 9.82.
XX    Oph |A symbiotic object featuring deep fadings
XX    Oph |of long duration [09489].
AH    Oph |H2O maser.
AQ    Oph |The chart in [06286] is wrong.
BE    Oph |The data in [00278] refer to another star.
BF    Oph |SB? P var? since JD2430000 - see Table.
BN    Oph |80d <= P <= 250d.
DM    Oph |P var. P = 220d (1893 - 1910), P = 216d (1914 - 1928).
DQ    Oph |P = 35d is possible.
FK    Oph |V2 (NGC 6273).
GM    Oph |V12 (NGC 6284).
GR    Oph |P var. Max = 2415425 + 136d*E (1893 - 1908);
GR    Oph |during 1910 - 1928 - see Table.
IL    Oph |P2 = 140d:.
IW    Oph |In the field of the globular cluster NGC 6293,
IW    Oph |possible cluster member.
KM    Oph |In the field of the globular cluster NGC 6304, field star.
KO    Oph |In a dark nebula.
KQ    Oph |P2 = 1500d.
KR    Oph |P2 > 5000d.
OU    Oph |V70 (NGC 6266).
PU    Oph |VB (A = V29 (NGC 6266), the data are in the Table; B = V28
PU    Oph |(NGC 6266), 16.6m - 17m, 4B, 4.8", 7deg), B: RRAB,
PU    Oph |Max = 2433423.52 + 0.49749d*E, M - m = 0.15P.
V0378 Oph |Min II 14.2. In the region of the open cluster CR 359.
V0378 Oph |Epoch of Max is given.
V0380 Oph |Porb = 0.16d. Blue.
V0391 Oph |In the region of the open cluster CR 359. P var?
V0391 Oph |Before JD2427000 Min = 2425501.425 + 2.89558d*E [00432];
V0391 Oph |since JD2441500 - see Table.
V0392 Oph |Red.
V0402 Oph |P var. Max = 2425364 + 154d*E (JD2425350 - 670);
V0402 Oph |since JD2425670 - see Table.
V0413 Oph |Delta(S) = 3. Blazhko effect?
V0414 Oph |B - V: +0.41, +0.77.
V0423 Oph |In the region of the open cluster CR 359.
V0426 Oph |Outbursts separated by 17d - 55d [08079]; in 1976 - 77 the
V0426 Oph |cycle was 32.3d. Outside outbursts 12.7m - 13.3m, waves
V0426 Oph |with a cycle of 20 - 30 Min and slower variations.
V0438 Oph |H20 Maser.
V0439 Oph |B - V: +0.63, +0.97.
V0442 Oph |Porb = 0.14056d.
V0445 Oph |VB A (B 13.04m y, 21"nf). (k - b)2 = 0.35; Delta(S) = 2.
V0445 Oph |According to [05692], Blazhko effect (Pi > 2000d).
V0449 Oph |P var. Before JD243900 Min = 2428696.465 +
V0449 Oph |1.243078d*E; Min = 2442959.607 + 1.243095d*E
V0449 Oph |(JD2439000 - 43000); since JD2443000 - see Table.
V0451 Oph |Min II 8.31; Min II - Min I = 0.494P; DII = 0.12P.
V0452 Oph |Delta(S) = 5:.
V0455 Oph |P var? The Table gives mean elements which need
V0455 Oph |confirmation.
V0456 Oph |Min II 10.5. P var. Before JD2436100 Min =
V0456 Oph |2428422.341 + 1.015986d*E [00476]; since JD2441800 - see
V0456 Oph |Table.
V0465 Oph |B - V: +0.68, +1.10. P var?
V0471 Oph |Very red.
V0478 Oph |B - V: +0.86, +1.33. [A/H] = -0.7.
V0478 Oph |The elements need confirmation.
V0487 Oph |D <= 0.14P. In the region of the open cluster Cr 359.
V0496 Oph |In the region of the open cluster Cr 359.
V0501 Oph |Min II 11.1.
V0502 Oph |Min II 8.81. P var. Since JD2434500 - see Table.
V0506 Oph |Min II 12.0. In the region of the open cluster Cr 359.
V0508 Oph |Min II 10.59.
V0509 Oph |In the region of the open cluster Cr 359.
V0511 Oph |Min II 13.7. In the region of the open cluster Cr 359.
V0515 Oph |Max = 2425600 + 300d*E (JD2425600 - 26700); P = 140d
V0515 Oph |(JD2426700 - 27300); during JD2427300 - 30200 - see Table.
V0516 Oph |In the region of the globular cluster NGC 6304.
V0517 Oph |In the region of the globular cluster NGC 6304.
V0521 Oph |P = 164d (JD2415000 - 24600); P2 - 4000d.
V0526 Oph |Min II 13.6.
V0527 Oph |Min II 14.8.
V0532 Oph |P >= 6000d.
V0533 Oph |P >= 80d.
V0534 Oph |d = 0.03P.
V0535 Oph |d = 0.025P.
V0536 Oph |d = 0.04P:.
V0537 Oph |Min II 12.8.
V0540 Oph |d = 0.05P; Min II 13.4.
V0541 Oph |[A/H] = -1.0. In the region of the globular cluster
V0541 Oph |NGC 6401; cluster non-member?
V0543 Oph |Min II 13.6.
V0549 Oph |Min II 14.0.
V0550 Oph |Min II 13.0.
V0554 Oph |[A/H] = -1.1.
V0555 Oph |Sharp and flat maxima. Blazhko effect?
V0557 Oph |Min II 15.7. In the region of the open cluster Cr 359.
V0558 Oph |B - V: +0.57, +0.68. [Fe/H] = -1.48. According to [09037],
V0558 Oph |P = 0.299d.
V0564 Oph |[Fe/H] = -1.37. Epoch of Min is given. P var. Nonlinear
V0564 Oph |term: +0.0073d*(E + 10)**2.
V0565 Oph |P = 0.3957d is possible. Photoelectric observations of
V0565 Oph |1968 contradict the elements [05746].
V0566 Oph |dI = 0.048P; Min II 7.89, dII = 0.06P. P var. Before
V0566 Oph |JD2440500 Min = 2436744.4200 + 0.40964091d*E [08287]; since
V0566 Oph |JD2440500 - see Table.
V0567 Oph |(k - b)2 = 0.22; Delta(S) = 0. According to [07984],
V0567 Oph |Max = 2441134.467 + 0.1300729d*E.
V0568 Oph |Red.
V0570 Oph |VB A (B 16.3m, 5", 90deg).
V0572 Oph |In the region of the open cluster Cr 359.
V0573 Oph |d = 0.034P. In the region of the open cluster Cr 359.
V0574 Oph |P2 ~500d.
V0577 Oph |Min II 11.9. Min II - Min I = 0.583P. DII = 0.050P.
V0577 Oph |e = 0.22.
V0580 Oph |VB A (B 15.5m, 0.2').
V0585 Oph |A long-period variation is superimposed?
V0586 Oph |In the region of the open cluster Cr 359.
V0590 Oph |Min II 13.6.
V0592 Oph |Max = 2427227 + 78d*E (JD2426100 - 29400);
V0592 Oph |during JD2429400 - 30150 - see Table.
V0592 Oph |After intervals of irregular variability the periodicity
V0592 Oph |resumes without phase shift.
V0605 Oph |Epoch of Min is given.
V0618 Oph |Min II 14.7:.
V0636 Oph |d = 0.030P.
V0683 Oph |P var. The light curve shape varies.
V0687 Oph |P may be twice longer.
V0693 Oph |Blazhko effect? [05692].
V0695 Oph |P var? The light curve shape varies.
V0698 Oph |P var? since JD2442950 - see Table.
V0700 Oph |B - V: +0.49, +0.50. [Fe/H] = -2.10.
V0716 Oph |Delta(S) = 7.
V0720 Oph |VI (NGC 6171). Cluster non-member.
V0722 Oph |P var. Max = 2437089.456 + 0.6190385d (JD2419900 - 37100)
V0722 Oph |[07806]; since JD2436700 - see Table.
V0729 Oph |P var. Max = 2437492.766 + 0.4685794d*E (JD2423500 - 37800)
V0729 Oph |[03560]; since JD2437400 - see Table.
V0732 Oph |Unusual light curve (sharp Max; primary Min; broad Max;
V0732 Oph |secondary Min 15.2).
V0734 Oph |P var. Max = 2420636.497 + 0.562489d*E (JD2420600 -
V0734 Oph |29100); during JD2429100 - 37150 - see Table.
V0735 Oph |Min II 10.6.
V0737 Oph |P = 374d is possible.
V0767 Oph |According to [00104], waves with Delta(m) = 0.3m - 1.4m vis
V0767 Oph |of 50d - 110d duration; mean brightness var,
V0767 Oph |Delta(m) ~0.4m in 800d - 1000d.
V0782 Oph |Very red.
V0784 Oph |B - V: +0.26, +0.56. The period should be checked.
V0786 Oph |Red.
V0788 Oph |Blazhko effect? Pi = 115d.
V0799 Oph |P = 215d is possible.
V0802 Oph |Red.
V0816 Oph |B - V: +0.25, +0.63.
V0822 Oph |Blazhko effect?
V0823 Oph |In the region of the open cluster IC 4665.
V0825 Oph |In the region of the open cluster IC 4665.
V0829 Oph |Blazhko effect? Pi = 165d.
V0832 Oph |Red.
V0838 Oph |P2 ~500d is possible.
V0839 Oph |mu = 0.041", ro = 292deg. Min II 9.38.
V0840 Oph |VB A (B 12m, 16", 116deg).
V0841 Oph |Max = 2396146.
V0843 Oph |SN Kepler. Max 2307193. Gaseous remnant.
V0844 Oph |Min II 14.9.
V0845 Oph |VB A (B 15.7m).
V0847 Oph |Min II 13.1.
V0848 Oph |Min II 13.4.
V0851 Oph |Max = 2425828 + 95d*E (JD2425600 - 29700);
V0851 Oph |during JD2429700 - 34250 - see Table.
V0854 Oph |According to [08116], the spectrum
V0854 Oph |resembles that of a T Tau - type star.
V0868 Oph |Min II 13.6. In the region of the open cluster Cr 359.
V0870 Oph |In the region of the open cluster Cr 359.
V0872 Oph |P = 0.825d is possible.
V0878 Oph |Min II 16.5. In the region of the open cluster Cr 359.
V0911 Oph |P2 = 81d, P3 = 114d. P4 > P3? Standstills up to 100d.
V0919 Oph |VB A (B sp).
V0920 Oph |Min II 15.9.
V0924 Oph |Min II 16.4.
V0929 Oph |d = 0.050P.
V0934 Oph |E type is possible.
V0936 Oph |In the region of the open cluster Cr 359.
V0938 Oph |Min II 15.3. In the region of the open cluster Cr 359.
V0940 Oph |Min II 15.6.
V0941 Oph |Min II 16.5.
V0943 Oph |Min II 16.4. In the region of the open cluster Cr 359.
V0945 Oph |Min II 15.1. In the region of the open cluster Cr 359.
V0947 Oph |Min II 14.5. In the region of the open cluster Cr 359.
V0952 Oph |P = 0.954d is possible.
V0954 Oph |In the region of the open cluster Cr 359. Min II 14.9.
V0954 Oph |According to [03500], const, V = 12.86m, B - V = +1.36m,
V0959 Oph |P var? Max = 2429785.419 + 0.084857d*E
V0959 Oph |(JD2429785 - 845) [02757]; during JD2443719 - 732 - see
V0959 Oph |Table; other possible elemente:
V0959 Oph |Max = 2443726.469 + 0.07786d*E.
V0960 Oph |In the region of the open cluster Cr 359.
V0963 Oph |Min II 15.1. In the region of the open cluster Cr 359.
V0968 Oph |[Fe/H] = -1.48. In the region of the open cluster Cr 359.
V0969 Oph |Min II 13.8:. In the region of the open cluster Cr 359.
V0977 Oph |In the region of the globular cluster NGC 6426.
V0978 Oph |In the region of the globular cluster NGC 6426.
V0979 Oph |V11 (NGC 6426). Cluster non-member.
V0980 Oph |In the the region of globular cluster NGC 6426.
V0980 Oph |P = 0.25740d is possible.
V0983 Oph |In the region of the open cluster Cr 359.
V0986 Oph |In July 1980 Vr varied with P = 0.179d, 0.147d, 0.225d,
V0986 Oph |and possibly 0.097d, but there were no spectrum variations,
V0986 Oph |and the photometric P = 0.323d was not noticeable in Vr.
V0986 Oph |SB? Porb = 15d - 20d; there is also excess power
V0986 Oph |at low frequences in the photometric data. Earlier
V0986 Oph |studies revealed photometric periods 0.284d - 0.4d
V0986 Oph |and violation of periodicity.
V0987 Oph |d = 0.02P. Min II 14.6. In the region of the open cluster
V0987 Oph |Cr 359.
V0998 Oph |In the region of the globular cluster NGC 6171.
V0999 Oph |In the region of the globular cluster NGC 6171.
V1000 Oph |Blazhko effect?
V1002 Oph |Min II 15.2.
V1002 Oph |RRC type with twice shorter P is possible.
V1004 Oph |Blazhko effect?
V1010 Oph |Min II 6.46. P var. P = 0.661464d (JD2415000 - 25000)
V1010 Oph |[05738]; since JD2425000 - see Table, nonlinear term:
V1010 Oph |-3.87d*10**(-10)*E**2. Min I var.The light curve shape and
V1010 Oph |the depth of Min I var.
V1011 Oph |Blazhko effect?
V1015 Oph |D <= 0.23P, d < 0.02P; Min II 14.5.
V1017 Oph |[Fe/H] = -1.25. P var? Max = 2437433.935 + 0.2343d*E
V1017 Oph |(JD2437433 - 514) [03625]. During
V1017 Oph |JD2442954 - 45140 - see Table.
V1017 Oph |According to [09037], P = 0.361d.
V1018 Oph |Possibly eclipsing.
V1021 Oph |Delta(m) var. B - V: +0.42, +0.62.
V1022 Oph |d = 0.06P:; Min II 15.95.
V1024 Oph |Max = 2437433.559 + 0.5914d*E (JD2437433 - 514)
V1024 Oph |[03625]. During JD2442954 - 45140 - see Table.
V1024 Oph |RR(B) type is possible; P = 0.371d satisfies the
V1024 Oph |observations during JD2442954 - 44407.
V1026 Oph |Max = 2437433.562 + 0.6563d*E (JD2437433 - 514)
V1026 Oph |[03625]. During JD2442954 - 45140 - see Table.
V1028 Oph |Blazhko effect?
V1032 Oph |P > 1.0d is not excluded.
V1033 Oph |Max = 2437433.714 + 0.4845d*E (JD2437433 - 514)
V1033 Oph |[03625]. During JD2442954 - 45140 - see Table.
V1035 Oph |Max = 2437433.388 + 0.6100d*E (JD2437433 - 514)
V1035 Oph |[03625]; during JD2442954 - 45140 - see Table.
V1039 Oph |P = 0.3166d is possible.
V1040 Oph |The light curve shape var.
V1041 Oph |[Fe/H] = -1.06.
V1042 Oph |The light curve shape var. Max = 2437433.633 + 0.5528d
V1042 Oph |(JD2437433 - 514) [03625]. During JD2442954 - 45140 - see
V1042 Oph |Table.
V1052 Oph |Max = 2437433.537 + 0.7546d*E (JD2437433 - 514)
V1052 Oph |[03625]; during JD2442954 - 45140 - see Table.
V1054 Oph |VB Wolf 630AB (A 9.76m V, 12.47mu; B 9.78m V; A = 0.22",
V1054 Oph |Porb = 1.71665 yr; C = Wolf 629, 11.70m V,14.75mu,
V1054 Oph |dM4, 72", D = vB8, 16.7m V, 221", common mu). mu = 1.19",
V1054 Oph |ro = 222deg. Lx/Lopt(V) = 0.05.
V1072 Oph |P var. Max = 2439025.31 + 0.444715d*E (JD2438500 - 39025);
V1072 Oph |since JD2442800 - see Table.
V1075 Oph |Red.
V1077 Oph |P var. Max = 2438614.40 + 0.373926d*E (JD2438200 - 700);
V1077 Oph |Max = 2442871.516 + 0.37384d*E (JD2442810 - 910):
V1077 Oph |Max = 2442983.345 + 0.373911d*E (JD2442920 - 3330);
V1077 Oph |since JD2443330 - see Table.
V1089 Oph |VB AB (B 16.4m, 2", 45deg).
V1099 Oph |Red.
V1100 Oph |Red.
V1111 Oph |OH, H2O, SiO maser.
V1120 Oph |Min II 14.3.
V1121 Oph |Soft X-ray source.
V1135 Oph |[Ca/H] = -0.74.
V1141 Oph |P var? The light curve shape var?
V1142 Oph |P var? The light curve shape var?
V1146 Oph |P = 185.2d is possible.
V1153 Oph |P = 153.0d is possible.
V1157 Oph |B - V: +0.42, +0.66.
V1161 Oph |P = 0.49d is possible [06438].
V1168 Oph |P var? The light curve shape var?
V1170 Oph |P = 360d: is possible [06438].
V1174 Oph |P var? The light curve shape var?
V1176 Oph |P = 269.0d is possible.
V1179 Oph |P var? The light curve shape var?
V1185 Oph |Other possible elements: Max = 2435630 + 177d*E [00001].
V1195 Oph |One more Max 2435637 (1956). Type M is possible.
V1203 Oph |P = 315d is possible [06438].
V1204 Oph |P = 144d: or P = 191d: are possible.
V1235 Oph |UV type is possible.
V1240 Oph |P = 0.42136d is possible.
V1244 Oph |The light curve shape var?
V1258 Oph |P var?
V1261 Oph |The light curve is not typical for the P in the Table [06438].
V1262 Oph |The light curve is not typical for the P in the Table [06438].
V1276 Oph |[Ca/H] = -0.1.
V1296 Oph |[Ca/H] = -0.9.
V1299 Oph |The light curve shape var?
V1300 Oph |P = 235d: is possible.
V1305 Oph |Min II 17.9:.
V1307 Oph |The light curve shape var? Spurious period? [06438].
V1323 Oph |P var?
V1332 Oph |[Ca/H] = -0.64.
V1348 Oph |The light curve shape var?
V1355 Oph |The light curve shape var?
V1403 Oph |P = 215d?
V1423 Oph |The light curve shape var?
V1426 Oph |P var?
V1451 Oph |P = 179.4d?
V1474 Oph |P = 127d:?
V1491 Oph |P = 328.0d?
V1492 Oph |The light curve shape var?
V1505 Oph |P = 86d:?
V1512 Oph |The light curve shape var?
V1526 Oph |P = 0.29745d?
V1532 Oph |P = 144.4d?
V1534 Oph |P = 198.8d?
V1548 Oph |The minor planet (336) Lacadiera.
V1554 Oph |P = 136.0d?
V1568 Oph |P = 275.5d?
V1571 Oph |P var?
V1573 Oph |Type E?
V1583 Oph |P - spurious?
V1616 Oph |Type E?
V1628 Oph |The light curve shape var?
V1637 Oph |[Ca/H] = -0.44.
V1661 Oph |The light curve shape var?
V1666 Oph |P = 154.2d?
V1676 Oph |Close optical companion?
V1682 Oph |P = 118.0d?
V1687 Oph |Type CW?
V1702 Oph |P = 121d?
V1705 Oph |P var?
V1710 Oph |P = 0.37422d?
V1731 Oph |The light curve shape var?
V1736 Oph |P = 143.8d?, P = 244.5d?
V1744 Oph |P = 191.6d?
V1748 Oph |A var. Type CW?
V1754 Oph |P = 128.4d?
V1768 Oph |The light curve shape var?
V1775 Oph |Type EW?
V1793 Oph |P = 170d:?
V1803 Oph |The star is not SVS 438.
V1805 Oph |The light curve shape var?
V1811 Oph |Min II 17.9:.
V1814 Oph |P = 160.4d?
V1822 Oph |P var?
V1829 Oph |P = 143.2d?
V1840 Oph |V 12 (NGC 6333 = M9). Cluster member.
V1841 Oph |The light curve shape var?
V1845 Oph |V7 (NGC 6333 = M9). Cluster member.
V1853 Oph |The light curve shape var?
V1860 Oph |[Ca/H] = -0.49.
V1861 Oph |P = 142.0d?
V1864 Oph |V3 (NGC 6333 = M9). Cluster member.
V1886 Oph |The light curve shape var?
V1889 Oph |P = 316.0d?
V1895 Oph |The light curve shape var?
V1905 Oph |P = 149.0d?
V1919 Oph |P = 102.8d?, P = 227.0d?
V1939 Oph |P = 330.0d?
V1946 Oph |The light curve shape var?
V1952 Oph |P = 248.0d?
V1953 Oph |P = 199d:?, P = 235d:?
V1954 Oph |P = 159.6d?
V1973 Oph |P = 0.24154d?
V1989 Oph |A var?
V1990 Oph |P = 121d:?
V1991 Oph |The light curve shape var?
V1994 Oph |P = 170.0d?
V1998 Oph |P = 270.5d?
V2002 Oph |The light curve shape var?
V2003 Oph |[Ca/H] = -0.96.
V2009 Oph |V5 (NGC 6356). Cluster member.
V2010 Oph |[CA/H] = -0.79.
V2016 Oph |[CA/H] = -0.96.
V2042 Oph |P var. Max = 2430146.478 + 0.5385d*E (JD2429100 -
V2042 Oph |30202); since JD2436700 - see Table.
V2045 Oph |The chart in [05159] is wrong.
V2048 Oph |SB2 [06598]. In the region of the open cluster Cr 359.
V2048 Oph |Along with irregular light variations typical for be stars
V2048 Oph |there are rapid flares with the amplitudes up to 1.8m
V2048 Oph |(lambda eff = 5800 A) [06150]. It is not excluded that the
V2048 Oph |flares occur on a fainter companion of the system.
V2051 Oph |Usually - 15.0m with strong flickering of brightness
V2051 Oph |(up to 0.4m is 5 minutes) and rare flares. At the same
V2051 Oph |time the eclipses are observed with depth to 2.5m with the
V2051 Oph |elements: Min = 2444787.32124 + 0.062427865d*E [09550];
V2051 Oph |D = 0.0088P:, d = 0.0065P.
V2058 Oph |In the dark nebula in the rho Oph region.
V2059 Oph |In the dark nebula in the rho Oph region.
V2061 Oph |In the region of the globular cluster NGC 6171 (M 107).
V2062 Oph |In the dark nebula in the rho Oph region.
V2063 Oph |The minor planet (64) Angelina.
V2064 Oph |In the dark nebula in the rho Oph region.
V2101 Oph |In a dark nebula.
V2102 Oph |In the region of the globular cluster NGC 6293.
V2105 Oph |Vr = 100 km/s.
V2106 Oph |<Vr> = -102 km/s.
V2108 Oph |H2O, SiO maser.
V2112 Oph |The primary oscillation with A1 = 0.0172m
V2112 Oph |(see Table) is superimposed by the secondary one
V2112 Oph |(A2 = 0.0061m) with the elements:
V2112 Oph |Max = 2444114.531: + 0.1449461d*E.
V2116 Oph |X-ray pulsar. The pulse period is decreasing: 135s (1971),
V2116 Oph |112.076s (1979), 109.668s (1980) [09553]. The spin-period
V2116 Oph |may be twice longer.
V2118 Oph |Probably rapidly rotating single spotted F type star.
V2118 Oph |Max brightness epoch is given.
V2119 Oph |In the region of the globular cluster
V2119 Oph |NGC 6284. Not a member of the cluster.
V2120 Oph |V6 (NGC 6284). In the region of the globular cluster
V2120 Oph |NGC 6284. Not a member of the cluster.
V2121 Oph |V10 (NGC 6284). In the region of the globular cluster
V2121 Oph |NGC 6284. Not a member of the cluster.
V2122 Oph |In the region of the globular cluster NGC 6284. Not
V2122 Oph |a member of the cluster.
V2123 Oph |V11 (NGC 6284). In the region of the globular cluster
V2123 Oph |NGC 6284. Not a member of the cluster.
V2124 Oph |In the region of the globular cluster NGC 6284. Not
V2124 Oph |a member of the cluster.
V2391 Oph |Porb = 88.13yr. Component B is a suspected variable star
V2391 Oph |(NSV 24260) and may be the cause of variations.
V2561 Oph |Not a supernova.
tet   Oph |SB1 (Porb = 11.44d [06597]).
tet   Oph |The basic oscillation (see Table) is superimposed by
tet   Oph |oscillations with the periods: P1 = 0.092551d,
tet   Oph |P2 = 0.069452d, P3 = 0.0555d, P4 = 0.0464d, P02 =
tet   Oph |0.137255d, P13 = 0.13845d, P24 = 0.13990d, P03 = 0.09185d.
khi   Oph |SB 1 (Porb = 138.8d [09558]).
ome   Oph |P = 1.5d?
R     Ori |SC 5/9.5 E. P var. Max = 2399420 + 378d*E
R     Ori |(JD2395600 - 99500); Max = 2412687 + 378.1d*E
R     Ori |(JD2403200 - 12700); Max = 2414230 + 366.5d*E
R     Ori |(JD2413800 - 16800); Max = 2417943 + 378.1d*E
R     Ori |(JD2416800 - 21350); Max = 2421352 + 384.9d*E
R     Ori |(JD2421350 - 24100); since JD2424100 - see Table.
S     Ori |VB A (B 10.9m, 47", 228deg). SiO maser. P var.
S     Ori |Max = 2404538 + 412.00d*E (JD2404520 - 13600);
S     Ori |Max = 2414014 + 427.15d*E (JD2414000 - 19150);
S     Ori |Max = 2419567 + 416.11d*E (JD2419570 - 22890);
S     Ori |Max = 2423312 + 407.10d*E (JD2423320 - 31050);
S     Ori |Max = 2431454 + 438.53d*E (JD2431500 - 39000)
S     Ori |[03765]; since JD2439000 - see Table.
T     Ori |In the T-association of the Orion nebula. Connected with
T     Ori |a cometary nebula.
U     Ori |SiO, OH, H2O maser. P var. Max = 2409881 + 374.5d*E
U     Ori |(JD2409800 - 15900); Max = 2415871 + 367.9d*E
U     Ori |(JD2415900 - 21000); Max = 2421016 + 376.0d*E
U     Ori |(JD2421000 - 29300); Max = 2428164 + 368.3d*E
U     Ori |(JD2428100 - 32900) [00960];
U     Ori |Max = 2433336 + 372.7d*E (JD2432900 - 43800);
U     Ori |since JD2443800 - see Table.
V     Ori |P var. Max = 2413656 + 264.8d*E (JD2411800 - 18700);
V     Ori |Max = 2418987 + 271.7d*E (JD2418700 - 24600);
V     Ori |Max = 2424695 + 263.7d*E (JD2424600 - 29400)
V     Ori |[00960]; Max = 2430769 + 269.9d*E (JD2430700 - 36200);
V     Ori |since JD2437700 - see Table.
W     Ori |Mean magnitude varies with P = 2450d.
Z     Ori |Min II 9.9; d = 0.013P.
RS    Ori |P var. Max = 2428073.205 + 7.566836d*E (JD2416500 -
RS    Ori |33000); since JD2435000 - see Table.
RT    Ori |Mean magnitude varies with P = 3200d.
RU    Ori |In the region of the nebula IC 434.
RV    Ori |In the region of the nebula IC 434.
RW    Ori |In the region of the nebula IC 434.
RX    Ori |In the region of the Orion nebula T-association.
RZ    Ori |In the region of the Orion nebula T-association.
SS    Ori |In the region of the Orion nebula T-association.
ST    Ori |In the region of the Orion nebula T-association.
SU    Ori |In the region of the Orion nebula T-association.
SV    Ori |In the region of the Orion nebula T-association.
SW    Ori |In the region of the Orion nebula T-association.
SX    Ori |In the region of the Orion nebula T-association.
SY    Ori |In the region of the Orion nebula T-association.
SZ    Ori |In the region of the Orion nebula T-association.
TT    Ori |In the region of the Orion nebula T-association.
TU    Ori |In the region of the Orion nebula T-association.
TV    Ori |In the region of the Orion nebula T-association.
TW    Ori |In the region of the Orion nebula T-association.
TX    Ori |VB A (B = TY Ori, 42.4", 45deg); in the region of
TX    Ori |the nebula IC 434.
TY    Ori |VB B (A = TX Ori); in the region of the nebula IC 434.
TZ    Ori |In the region of the nebula IC 434.
UW    Ori |Min II 11.6.
UY    Ori |In the region of the Orion nebula T-association.
UZ    Ori |In the region of the Orion nebula T-association.
VV    Ori |Min II 5.50; dI = 0.055P; dII = 0.064P.
VV    Ori |There is third component in the system
VV    Ori |(Porb = 119.09d [08045]).
VW    Ori |In the region of the Orion nebula T-association.
VX    Ori |In the region of the Orion nebula T-association.
VY    Ori |VB A (B = 16.6mV, 16", 135deg). In the region of the Orion
VY    Ori |nebula T-association.
VZ    Ori |In the region of the Orion nebula T-association.
WW    Ori |In the region of the Orion nebula T-association.
WX    Ori |VB A (B 17m, 11", 10deg). In the region of the Orion nebula
WX    Ori |T-association.
WY    Ori |In the region of the Orion nebula T-association.
WZ    Ori |In the region of the Orion nebula T-association.
XX    Ori |In the region of the Orion nebula T-association.
XY    Ori |In the region of the Orion nebula T-association.
XZ    Ori |The periodicity in light variations is possible.
XZ    Ori |In the region of the Orion nebula T-association.
YY    Ori |Emission. In the region of the Orion nebula T-association.
YZ    Ori |In the region of the Orion nebula T-association.
ZZ    Ori |In the region of the Orion nebula T-association.
AA    Ori |In the region of the Orion nebula T-association.
AB    Ori |In the region of the Orion nebula T-association.
AC    Ori |In the region of the Orion nebula T-association.
AE    Ori |In the region of the Orion nebula T-association.
AF    Ori |In the region of the Orion nebula T-association.
AG    Ori |VB A (B 16.4mV, 16", 185deg). In the region of the Orion
AG    Ori |nebula T-association.
AH    Ori |In the region of the Orion nebula T-association.
AI    Ori |In the region of the Orion nebula T-association.
AK    Ori |In the region of the Orion nebula T-association.
AL    Ori |In the region of the Orion nebula T-association.
AM    Ori |VB A (B 20.3mV, 3.5", 320deg). In the region of the Orion
AM    Ori |nebula T-association.
AN    Ori |In the region of the Orion nebula T-association.
AO    Ori |In the region of the Orion nebula T-association.
AP    Ori |In the region of the Orion nebula T-association.
AQ    Ori |In the region of the Orion nebula T-association.
AR    Ori |VB A (B 2", 240deg). In the region of the Orion nebula
AR    Ori |T-association.
AS    Ori |In the region of the Orion nebula T-association.
AT    Ori |In the region of the Orion nebula T-association.
AU    Ori |In the region of the Orion nebula T-association.
AV    Ori |VB A (B 18.7mV, 6", 305deg). In the region of the nebula
AV    Ori |T-association.
AW    Ori |In the region of the Orion nebula T-association.
AX    Ori |In the region of the Orion nebula T-association.
AY    Ori |In the region of the Orion nebula T-association.
AZ    Ori |In the region of the Orion nebula T-association.
BB    Ori |In the region of the Orion nebula T-association.
BC    Ori |In the region of the Orion nebula T-association.
BD    Ori |In the region of the Orion nebula T-association.
BE    Ori |In the region of the Orion nebula T-association.
BF    Ori |In the region of the Orion nebula T-association.
BG    Ori |In the region of the nebula IC 434.
BH    Ori |In the region of the Orion nebula T-association.
BK    Ori |P var. Max = 2422016 + 338.0d*E (JD2413550 - 22100);
BK    Ori |Max = 2428880 + 326.5d*E (JD2422300 - 28880);
BK    Ori |Max = 2429940 + 345.3d*E (JD2428880 - 29940);
BK    Ori |Max = 2432892 + 327.7d*E (JD2429940 - 32900);
BK    Ori |Max = 2438800 + 346.3d*E (JD2432900 - 38800);
BK    Ori |since JD2438800 - see Table.
BM    Ori |In the region of the Orion nebula T-association. In the
BM    Ori |cluster NGC 1976. Orion Trapezium
BM    Ori |member: teta**1 Ori B (A = V1016 Ori; B 8.7", 32deg;
BM    Ori |C 5.13m, 13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.05P;
BM    Ori |Min II 7.98. Shape of the light curve and depths of minima
BM    Ori |vary.
BO    Ori |In the region of the Orion nebula T-association.
BP    Ori |In the region of the Orion nebula T-association.
BS    Ori |In the region of the Orion nebula T-association.
BT    Ori |In the region of the Orion nebula T-association.
BU    Ori |In the region of the Orion nebula T-association.
BV    Ori |In the region of the Orion nebula T-association.
BW    Ori |In the region of the Orion nebula T-association.
BX    Ori |In the region of the Orion nebula T-association.
BY    Ori |In the region of the Orion nebula T-association.
BZ    Ori |In the region of the Orion nebula T-association.
CC    Ori |In the region of the Orion nebula T-association.
CD    Ori |In the region of the Orion nebula T-association.
CE    Ori |In the region of the Orion nebula T-association.
CF    Ori |In the region of the Orion nebula T-association.
CG    Ori |In the region of the Orion nebula T-association.
CH    Ori |In the region of the Orion nebula T-association.
CI    Ori |VB A (B 9.70m, 12.9", 88deg).
CM    Ori |P var?
CN    Ori |Porb = 0.163097d.
CN    Ori |Light curve is superposed by oscillations with
CN    Ori |the following elements: Max0 = 2444941.5032 +
CN    Ori |0.163097d*E (A0 = 0.2m), Max1 = 2444941.573 +
CN    Ori |0.15946d*E (A1 = 0.1m) [09471].
CN    Ori |Sometimes smaller rapid light oscillations are also
CN    Ori |observed with periods 24.3s - 29.5s (A<1%).
CO    Ori |Member of the T-association
CO    Ori |CO Ori. VB A (B 13m, 1", 280deg).
CP    Ori |Min II 11.2. P var [02545].
CT    Ori |SRD? P = 68d? [09496].
CW    Ori |Min II 13.2.
DK    Ori |In the region of the Orion nebula T-association.
DK    Ori |VB (ro < 3").
DL    Ori |In the region of the Orion nebula T-association.
DM    Ori |In the region of the Orion nebula T-association.
DN    Ori |Min II 9.9; d = 0.026P. P var. Min I = 2428497.51 +
DN    Ori |12.9649d*E (JD2425200 - 28600); since
DN    Ori |JD2435570 - see Table.
DY    Ori |B - V: +0.58, +1.72.
EG    Ori |d = 0.086P. P var?
EQ    Ori |Min II 10.3. P var. Min I = 2425889.706 + 1.74608d*E
EQ    Ori |(JD2425600 - 26700) [02839]; Min I = 2429219.467 +
EQ    Ori |1.74611d*E (JD2427700 - 31000) [00001];
EQ    Ori |since JD2431000 - see Table.
ER    Ori |VB A (B 13.6", 0deg). Min II 9.97. P var. Min I =
ER    Ori |2426336.6485 + 0.4233955d*E (JD2426330 - 33920)
ER    Ori |[00279]; Min I = 2434765.6306 + 0.42340620d*E
ER    Ori |(JD2433920 - 35475) [02278]; Min I = 2436508.7851 +
ER    Ori |0.4234009d*E (JD2435475 - 40000) [03787];
ER    Ori |since JD2440000 - see Table. Shape of the light curve
ER    Ori |varies.
ET    Ori |Min II 11.3. P var?
EW    Ori |Min II 10.5; Min II - Min I = 0.529P.
EW    Ori |In the region of the open cluster CR 70.
EW    Ori |In [00007] Min II are accepted to be Min I, and vice
EW    Ori |versa (Min II - Min I = 0.47P).
EW    Ori |For decisive choice of the Min I epoch photoelectric
EW    Ori |observations are necessary. P var? Min II =
EW    Ori |2429974.810 + 6.9368005d*E [00007]; since
EW    Ori |JD2430000 - see Table.
EY    Ori |Min II 9.54; d = 0.003P. In the region of the Orion
EY    Ori |nebula T-association. P var.
EY    Ori |Min I = 2427310.420 + 16.787450d*E [00007];
EY    Ori |since JD2427500 - see Table.
EZ    Ori |In the region of the Orion nebula T-association.
FF    Ori |Min II 10.3.
FH    Ori |d = 0.035P. P var.
FI    Ori |VB A (B 10.5m, 5", 323deg).
FI    Ori |Shape of the light curve varies, probably periodically
FI    Ori |[03790,05475].
FK    Ori |P var. Min = 2427773.390 + 1.947447d*E (JD2426900 -
FK    Ori |37500); since JD2437500 - see Table.
FL    Ori |P var. Min = 2427452.271 + 1.550971d*E (JD2427450 -
FL    Ori |29600) [03115]; Min = 2430400.649 + 1.55093d*E
FL    Ori |(JD2429600 - 30400);Min = 2432517.755 + 1.550991d*E
FL    Ori |(JD2430400 - 32900); Min = 2434459.571 + 1.550965d*E
FL    Ori |(JD2432900 - 35050); Min = 2436649.568 + 1.550995d*E
FL    Ori |(JD2435050 - 40600); since JD2440600 - see Table.
FO    Ori |Min II 9.7; d = 0.005P.
FR    Ori |Min II 11.1.
FT    Ori |Min II 9.60; DII = 0.08P; Min II - Min I = 0.73P. P var.
FT    Ori |Min I = 2433009.553 + 3.150404d*E (JD2426380 - 38000)
FT    Ori |[02758]; since JD2438000 - see Table.
FT    Ori |The period of apsidal motion 520 +- 100 years [07358].
FU    Ori |Member of FU Ori T-association. In the dark globule B35.
FU    Ori |Connected with a bright cometary nebula and the bright
FU    Ori |hydrogen nebula S 280. Light maximum was in summer
FU    Ori |1937. IN 1980 - 10.6m B.
FZ    Ori |Min II 11.2.
GG    Ori |Min II 11.1; Min II - Min I = 0.427P.
GP    Ori |SC 7/8- .
GQ    Ori |VB A (B 9.7m, 31", 324deg).
GW    Ori |In the T-association CO Ori.
GX    Ori |In the T-association CO - Ori.
GY    Ori |In the T-association CO - Ori.
GZ    Ori |In the region of the Orion nebula T-association.
HH    Ori |In the region of the Orion nebula T-association.
HI    Ori |In the T-association CO - Ori.
HK    Ori |In the T-association CO - Ori.
HK    Ori |Connected with a bright cometary nebula. CO, CH, OH
HK    Ori |emission.
HL    Ori |In the region of the Orion nebula T-association.
HM    Ori |In the T-association CO - Ori.
HN    Ori |In the region of the Orion nebula T-association.
HO    Ori |In the region of the Orion nebula T-association.
HP    Ori |In the region of the Orion nebula T-association.
HQ    Ori |In the region of the Orion nebula T-association.
HR    Ori |In the region of the Orion nebula T-association.
HS    Ori |In the region of the Orion nebula T-association.
HT    Ori |In the region of the Orion nebula T-association.
HU    Ori |In the region of the Orion nebula T-association.
HV    Ori |In the region of the Orion nebula T-association.
HW    Ori |In the region of the Orion nebula T-association.
HX    Ori |In the region of the Orion nebula T-association.
HY    Ori |In the region of the Orion nebula T-association.
HZ    Ori |In the region of the Orion nebula T-association.
II    Ori |In the region of the Orion nebula T-association.
IK    Ori |In the region of the Orion nebula T-association.
IL    Ori |In the region of the Orion nebula T-association.
IM    Ori |In the region of the Orion nebula T-association.
IN    Ori |In the region of the Orion nebula T-association.
IO    Ori |In the region of the Orion nebula T-association.
IP    Ori |In the region of the Orion nebula T-association.
IQ    Ori |In the region of the Orion nebula T-association.
IR    Ori |In the region of the Orion nebula T-association.
IS    Ori |In the region of the Orion nebula T-association.
IT    Ori |In the region of the Orion nebula T-association.
IU    Ori |In the region of the Orion nebula T-association.
IV    Ori |In the region of the Orion nebula T-association.
IW    Ori |In the region of the Orion nebula T-association.
IX    Ori |In the region of the Orion nebula T-association.
IY    Ori |In the region of the Orion nebula T-association.
IZ    Ori |In the region of the Orion nebula T-association.
KK    Ori |In the region of the Orion nebula T-association.
KL    Ori |In the region of the Orion nebula T-association.
KM    Ori |In the region of the Orion nebula T-association.
KN    Ori |In the region of the Orion nebula T-association.
KO    Ori |In the region of the Orion nebula T-association.
KP    Ori |In the region of the Orion nebula T-association.
KQ    Ori |In the region of the Orion nebula T-association.
KR    Ori |In the region of the Orion nebula T-association.
KS    Ori |In the region of the Orion nebula T-association.
KT    Ori |In the region of the Orion nebula T-association.
KU    Ori |In the region of the Orion nebula T-association.
KV    Ori |In the region of the Orion nebula T-association.
KW    Ori |In the region of the Orion nebula T-association.
KX    Ori |In the region of the Orion nebula T-association.
KY    Ori |In the region of the Orion nebula T-association.
KZ    Ori |In the region of the Orion nebula T-association.
LL    Ori |In the region of the Orion nebula T-association.
LM    Ori |In the region of the Orion nebula T-association.
LN    Ori |In the region of the Orion nebula T-association.
LO    Ori |In the region of the Orion nebula T-association.
LP    Ori |In the region of the Orion nebula T-association.
LQ    Ori |In the region of the Orion nebula T-association.
LR    Ori |In the region of the Orion nebula T-association.
LS    Ori |In the region of the Orion nebula T-association.
LT    Ori |In the region of the Orion nebula T-association.
LU    Ori |In the region of the Orion nebula T-association.
LV    Ori |In the region of the Orion nebula T-association.
LW    Ori |In the region of the Orion nebula T-association.
LX    Ori |In the region of the Orion nebula T-association.
LY    Ori |In the region of the Orion nebula T-association.
LZ    Ori |VB B (A 10.3m; B 14.1", 219deg). In the region of the
LZ    Ori |Orion nebula T-association.
MM    Ori |In the region of the Orion nebula T-association.
MN    Ori |In the region of the Orion nebula T-association.
MO    Ori |In the region of the Orion nebula T-association.
MP    Ori |In the region of the Orion nebula T-association.
MQ    Ori |In the region of the Orion nebula T-association.
MR    Ori |In the region of the Orion nebula T-association.
MS    Ori |In the region of the Orion nebula T-association.
MT    Ori |In the region of the Orion nebula T-association.
MU    Ori |In the region of the Orion nebula T-association.
MV    Ori |In the region of the Orion nebula T-association.
MW    Ori |In the region of the Orion nebula T-association.
MX    Ori |In the region of the Orion nebula T-association.
MY    Ori |In the region of the Orion nebula T-association.
MZ    Ori |In the region of the Orion nebula T-association.
NN    Ori |In the region of the Orion nebula T-association.
NO    Ori |In the region of the Orion nebula T-association.
NP    Ori |In the region of the Orion nebula T-association.
NQ    Ori |In the region of the Orion nebula T-association.
NR    Ori |In the region of the Orion nebula T-association.
NS    Ori |In the region of the Orion nebula T-association.
NT    Ori |In the region of the Orion nebula T-association.
NU    Ori |In the region of the Orion nebula T-association. In the
NU    Ori |nebula NGC 1982. Dust shell.
NV    Ori |In the region of the Orion nebula T-association.
NW    Ori |In the region of the Orion nebula T-association.
NX    Ori |In the region of the Orion nebula T-association.
NY    Ori |VB B (A = V566 Ori; B 5", 135deg). In the region of the
NY    Ori |Orion nebula T-association.
NZ    Ori |In the region of the Orion nebula T-association.
OO    Ori |In the region of the Orion nebula T-association.
OP    Ori |In the region of the Orion nebula T-association.
OQ    Ori |In the region of the Orion nebula T-association.
OR    Ori |In the region of the Orion nebula T-association.
OT    Ori |In the region of the Orion nebula T-association.
OU    Ori |In the region of the Orion nebula T-association.
OV    Ori |In the region of the Orion nebula T-association.
OW    Ori |In the region of the Orion nebula T-association.
OX    Ori |In the region of the Orion nebula T-association.
OY    Ori |In the region of the Orion nebula T-association.
OZ    Ori |In the region of the Orion nebula T-association.
PP    Ori |In the region of the Orion nebula T-association.
PQ    Ori |In the region of the nebula IC 434.
PR    Ori |In the region of the Orion nebula T-association.
PS    Ori |In the region of the Orion nebula T-association.
PT    Ori |In the region of the Orion nebula T-association.
PU    Ori |In the region of the nebula IC 434.
PV    Ori |In the region of the Orion nebula T-association.
PW    Ori |In the region of the Orion nebula T-association.
PX    Ori |<Vr> =  + 298 km/s [09511]. In the region of the Orion
PX    Ori |nebula T-association.
PY    Ori |In the region of the Orion nebula T-association.
PZ    Ori |In the region of the Orion nebula T-association.
QQ    Ori |In the region of the Orion nebula T-association.
QR    Ori |In the region of T-association FU Ori.
QT    Ori |P var? Elements given in the Table are valid in the
QT    Ori |interval JD2429640 - 35550.
V0340 Ori |Epoch of Min brightness is given.
V0343 Ori |Min II 11.0. Shape of the light curve and depth of
V0343 Ori |Min II vary.
V0347 Ori |In the region of the Orion nebula T-association.
V0348 Ori |In the region of the Orion nebula T-association.
V0349 Ori |In the region of the Orion nebula T-association.
V0353 Ori |In the region of the Orion nebula T-association.
V0354 Ori |In the region of the Orion nebula T-association.
V0355 Ori |In the region of the Orion nebula T-association.
V0356 Ori |In the region of the Orion nebula T-association.
V0357 Ori |In the region of the Orion nebula T-association.
V0358 Ori |In the region of the Orion nebula T-association.
V0359 Ori |In the region of the Orion nebula T-association.
V0359 Ori |Epoch of Min HEI line intensity is given.
V0359 Ori |According to [09512], P = 14.612d.
V0360 Ori |In the region of the Orion nebula T-association.
V0361 Ori |VB C (A 4.8m; B 6.1m, 52.4", 93deg; C 129", 97deg).
V0361 Ori |In the region of the Orion nebula T-association.
V0362 Ori |In the region of the Orion nebula T-association.
V0363 Ori |In the region of the Orion nebula T-association.
V0364 Ori |In the region of the Orion nebula T-association.
V0365 Ori |In the region of the Orion nebula T-association.
V0366 Ori |In the region of the Orion nebula T-association.
V0367 Ori |In the region of the Orion nebula T-association.
V0368 Ori |In the region of the Orion nebula T-association.
V0369 Ori |In the region of the Orion nebula T-association.
V0370 Ori |In the T-association CO - Ori.
V0371 Ori |mu = 0.28", ro = 238deg.
V0372 Ori |In the region of the Orion nebula T-association.
V0373 Ori |In the region of the Orion nebula T-association.
V0374 Ori |In the region of the Orion nebula T-association.
V0375 Ori |In the region of the Orion nebula T-association.
V0376 Ori |In the region of the Orion nebula T-association.
V0377 Ori |In the region of the Orion nebula T-association.
V0378 Ori |In the region of the Orion nebula T-association.
V0379 Ori |In the region of the Orion nebula T-association.
V0380 Ori |In the nebula NGC 1999. In the region of the Orion
V0380 Ori |nebula T-association. Spectrum description
V0380 Ori |[04002]. OH, CH emission.
V0381 Ori |In the region of the Orion nebula T-association.
V0382 Ori |P var. MAX = 2431146 + 227.8d*E (JD2429300 - 31200);
V0382 Ori |Mean period is given in the Table (JD2428100 - 33700).
V0383 Ori |In the region of the Orion nebula T-association.
V0384 Ori |In the region of the Orion nebula T-association.
V0385 Ori |In the region of the Orion nebula T-association.
V0386 Ori |In the region of the Orion nebula T-association.
V0387 Ori |In the region of the Orion nebula T-association.
V0388 Ori |In the region of the Orion nebula T-association.
V0389 Ori |In the region of the Orion nebula T-association.
V0390 Ori |In the region of the Orion nebula T-association.
V0391 Ori |In the region of the Orion nebula T-association.
V0393 Ori |In the region of the Orion nebula T-association.
V0394 Ori |In the region of the Orion nebula T-association.
V0395 Ori |In the region of the Orion nebula T-association.
V0396 Ori |In the region of the Orion nebula T-association.
V0397 Ori |In the region of the Orion nebula T-association.
V0398 Ori |In the region of the Orion nebula T-association.
V0399 Ori |In the region of the Orion nebula T-association.
V0400 Ori |In the region of the Orion nebula T-association.
V0401 Ori |In the region of the Orion nebula T-association.
V0402 Ori |In the region of the Orion nebula T-association.
V0403 Ori |In the region of the Orion nebula T-association.
V0404 Ori |In the region of the Orion nebula T-association.
V0405 Ori |In the region of the Orion nebula T-association.
V0406 Ori |In the region of the Orion nebula T-association.
V0407 Ori |In the region of the Orion nebula T-association.
V0408 Ori |In the region of the Orion nebula T-association.
V0409 Ori |In the region of the Orion nebula T-association.
V0410 Ori |In the region of the Orion nebula T-association.
V0411 Ori |In the region of the Orion nebula T-association.
V0412 Ori |In the region of the Orion nebula T-association.
V0413 Ori |In the region of the Orion nebula T-association.
V0414 Ori |In the region of the Orion nebula T-association.
V0415 Ori |In the region of the Orion nebula T-association.
V0416 Ori |In the region of the Orion nebula T-association.
V0417 Ori |In the region of the Orion nebula T-association.
V0418 Ori |In the region of the Orion nebula T-association.
V0419 Ori |In the region of the Orion nebula T-association.
V0420 Ori |In the region of the Orion nebula T-association.
V0421 Ori |In the region of the Orion nebula T-association.
V0422 Ori |In the region of the Orion nebula T-association.
V0423 Ori |In the region of the Orion nebula T-association.
V0424 Ori |In the region of the Orion nebula T-association.
V0425 Ori |In the region of the Orion nebula T-association.
V0426 Ori |In the region of the Orion nebula T-association.
V0427 Ori |In the region of the Orion nebula T-association.
V0428 Ori |In the region of the Orion nebula T-association.
V0432 Ori |Delta(S) = 0.
V0435 Ori |P var. Max = 2430350 + 186d*E (JD2429600 - 30730);
V0435 Ori |Max = 2431373 + 186d*E (JD2431370 - 3250) [02279];
V0435 Ori |since JD2434000 - see Table.
V0436 Ori |In the T-association CO Ori.
V0437 Ori |In the T-association CO Ori.
V0438 Ori |In the T-association CO Ori.
V0439 Ori |In the T-association CO Ori.
V0441 Ori |In the T-association CO Ori.
V0442 Ori |VB A (B 16.6m, 20", 73deg). In the T-association CO Ori.
V0443 Ori |In the T-association CO Ori.
V0444 Ori |In the T-association CO Ori.
V0445 Ori |In the T-association CO Ori.
V0446 Ori |In the T-association CO Ori.
V0447 Ori |In the T-association CO Ori.
V0448 Ori |In the T-association CO Ori.
V0449 Ori |In the T-association CO Ori.
V0449 Ori |In [08289] was considered as an EW type variable with the
V0449 Ori |elements: Min I = 2430259.622 + 0.441990d*E
V0449 Ori |(JD2430250 - 5550), 14.8m - 15.7m pg.
V0450 Ori |In the T-association CO Ori.
V0452 Ori |In the T-association CO Ori.
V0453 Ori |In the T-association CO Ori.
V0454 Ori |In the T-association CO Ori.
V0455 Ori |In the T-association CO Ori.
V0456 Ori |In the T-association CO Ori.
V0457 Ori |In the T-association CO Ori.
V0458 Ori |In the T-association CO Ori.
V0460 Ori |In the T-association CO Ori.
V0461 Ori |In the T-association CO Ori.
V0463 Ori |In the T-association CO Ori.
V0464 Ori |In the T-association CO Ori.
V0465 Ori |In the T-association CO Ori.
V0466 Ori |In the region of the Orion nebula T-association.
V0467 Ori |In the T-association CO Ori.
V0468 Ori |In the region of the Orion nebula T-association.
V0470 Ori |In the region of the Orion nebula T-association. Star
V0470 Ori |Pi 1411. Near to WY Ori = Pi 1396.
V0473 Ori |In the region of the Orion nebula T-association.
V0474 Ori |In the region of the Orion nebula T-association.
V0475 Ori |In the region of the Orion nebula T-association.
V0476 Ori |In the region of the open cluster lambda Ori.
V0477 Ori |In the region of the open cluster lambda Ori.
V0478 Ori |In the region of the Orion nebula T-association.
V0479 Ori |In the region of the Orion nebula T-association. In the
V0479 Ori |infrared A>1.5m.
V0480 Ori |In the region of the Orion nebula T-association. In the
V0480 Ori |infrared A>1.5m.
V0481 Ori |In the region of the Orion nebula T-association.
V0482 Ori |In the region of the Orion nebula T-association.
V0484 Ori |In the region of the Orion nebula T-association.
V0484 Ori |In the infrared A>1.0m.
V0485 Ori |In the region of the Orion nebula T-association.
V0485 Ori |In the infrared  A>1.0m.
V0486 Ori |In the region of the Orion nebula T-association.
V0487 Ori |In the region of the Orion nebula T-association.
V0489 Ori |In the region of the Orion nebula T-association.
V0489 Ori |In the infrared A>1.0m.
V0490 Ori |In the region of the Orion nebula T-association.
V0490 Ori |In the infrared A>1.0m.
V0491 Ori |In the region of the Orion nebula T-association.
V0491 Ori |In the infrared A>1.0m.
V0492 Ori |In the region of the Orion nebula T-association.
V0492 Ori |Northern component of the close pair of infrared stars.
V0492 Ori |In the infrared A = 1m.
V0493 Ori |In the region of the Orion nebula T-association.
V0493 Ori |In the infrared A>1.0m.
V0494 Ori |In the region of the Orion nebula T-association.
V0495 Ori |In the region of the Orion nebula T-association.
V0495 Ori |Close binary (ro = 0.24"). It is unknown which of the
V0495 Ori |components varies.
V0496 Ori |In the region of the Orion nebula T-association.
V0496 Ori |In the infrared A>1.0m.
V0497 Ori |In the region of the Orion nebula T-association.
V0497 Ori |In the infrared A>1.0m.
V0498 Ori |In the region of the Orion nebula T-association.
V0500 Ori |In the region of the Orion nebula T-association.
V0501 Ori |In the region of the Orion nebula T-association.
V0502 Ori |In the region of the Orion nebula T-association.
V0504 Ori |Min II 15.4.
V0505 Ori |In the region of the nebula IC 434.
V0507 Ori |In the region of the nebula IC 434.
V0508 Ori |In the region of the nebula IC 434.
V0509 Ori |In the region of the nebula IC 434.
V0510 Ori |In the region of the nebula IC 434.
V0511 Ori |In the region of the nebula IC 434.
V0514 Ori |In the region of the nebula IC 434.
V0516 Ori |Max = 2430325 + 139d*E (JD2430250 - 5350); P = 70d
V0516 Ori |(JD2435350 - 550).
V0519 Ori |Min II 12.9.
V0522 Ori |In the region of the nebula IC 434.
V0523 Ori |In the region of the nebula IC 434.
V0525 Ori |Min II 14.7.
V0526 Ori |In the region of T-association FU Ori.
V0529 Ori |Nova Ori 1678?
V0529 Ori |Recurrent outburst was possibly observed at 1894 [02866].
V0529 Ori |Earlier the object was considered as nova Ori [1667
V0529 Ori |2862, 2863, 2867, 2868], its existence being considered
V0529 Ori |as doubtful [03813].
V0537 Ori |In the region of the open cluster lambda Ori.
V0538 Ori |In the region of the Orion nebula T-association.
V0539 Ori |In the region of the Orion nebula T-association.
V0540 Ori |In the region of the Orion nebula T-association.
V0541 Ori |In the region of the Orion nebula T-association.
V0542 Ori |In the region of the Orion nebula T-association.
V0544 Ori |In the region of the Orion nebula T-association.
V0545 Ori |In the region of the Orion nebula T-association.
V0546 Ori |In the region of the Orion nebula T-association.
V0547 Ori |In the region of the Orion nebula T-association.
V0548 Ori |In the region of the open cluster lambda Ori.
V0549 Ori |In the region of the open cluster lambda Ori.
V0550 Ori |In the region of the Orion nebula T-association.
V0551 Ori |In the region of the Orion nebula T-association.
V0552 Ori |In the region of the Orion nebula T-association.
V0553 Ori |In the region of the Orion nebula T-association.
V0554 Ori |In the region of the Orion nebula T-association.
V0555 Ori |In the region of the Orion nebula T-association.
V0556 Ori |In the region of the Orion nebula T-association.
V0557 Ori |In the region of the Orion nebula T-association.
V0559 Ori |In the region of the Orion nebula T-association.
V0560 Ori |In the region of the Orion nebula T-association.
V0561 Ori |In the region of the Orion nebula T-association.
V0562 Ori |In the region of the Orion nebula T-association.
V0563 Ori |In the region of the Orion nebula T-association.
V0564 Ori |In the region of the Orion nebula T-association.
V0565 Ori |In the region of the Orion nebula T-association.
V0566 Ori |In the region of the Orion nebula T-association.
V0567 Ori |In the region of the Orion nebula T-association.
V0568 Ori |In the region of the Orion nebula T-association.
V0569 Ori |In the region of the Orion nebula T-association.
V0570 Ori |In the region of the Orion nebula T-association.
V0571 Ori |In the region of the Orion nebula T-association.
V0572 Ori |In the region of the open cluster lambda Ori.
V0573 Ori |In the region of the Orion nebula T-association.
V0574 Ori |In the region of the Orion nebula T-association.
V0575 Ori |In the region of the Orion nebula T-association.
V0576 Ori |In the region of the Orion nebula T-association.
V0577 Ori |In the region of the Orion nebula T-association.
V0578 Ori |In the region of the Orion nebula T-association.
V0579 Ori |In the region of the Orion nebula T-association.
V0580 Ori |In the region of the Orion nebula T-association.
V0581 Ori |In the region of the Orion nebula T-association.
V0582 Ori |In the region of the Orion nebula T-association.
V0584 Ori |In the region of the Orion nebula T-association.
V0585 Ori |In the region of the Orion nebula T-association.
V0586 Ori |In the region of the Orion nebula T-association.
V0587 Ori |In the region of the Orion nebula T-association.
V0588 Ori |In the region of the Orion nebula T-association.
V0589 Ori |In the region of the Orion nebula T-association.
V0590 Ori |In the region of the Orion nebula T-association.
V0591 Ori |In the region of the Orion nebula T-association.
V0592 Ori |In the region of the Orion nebula T-association.
V0593 Ori |In the region of the Orion nebula T-association.
V0594 Ori |In the region of the Orion nebula T-association.
V0595 Ori |In the region of the nebula IC 434.
V0596 Ori |In the region of the open cluster lambda Ori.
V0597 Ori |In the region of the nebula IC 434.
V0598 Ori |In the region of the open cluster lambda Ori.
V0599 Ori |In the region of the Orion nebula T-association.
V0600 Ori |In the region of the nebula IC 434.
V0601 Ori |In the region of the nebula IC 434.
V0602 Ori |In the region of the nebula IC 434.
V0603 Ori |In the region of the nebula IC 434.
V0604 Ori |In the region of the nebula IC 434.
V0605 Ori |In the region of the nebula IC 434.
V0606 Ori |In the region of the nebula IC 434.
V0607 Ori |In the region of the nebula IC 434.
V0608 Ori |In the region of the nebula IC 434.
V0610 Ori |In the region of the nebula IC 434.
V0611 Ori |In the region of the nebula IC 434.
V0612 Ori |VB, SE-comp.; NW-comp.=NSV 02555. In the region of the
V0612 Ori |nebula IC 434.
V0614 Ori |In the region of T-association FU Ori.
V0615 Ori |In the region of the nebula IC 434.
V0616 Ori |In the region of the nebula IC 434.
V0617 Ori |In the region of the nebula IC 434.
V0618 Ori |In the region of the nebula IC 434.
V0619 Ori |In the region of the nebula IC 434.
V0620 Ori |In the region of the nebula IC 434.
V0621 Ori |In the region of the nebula IC 434.
V0622 Ori |In the region of the nebula IC 434.
V0623 Ori |In the region of the nebula IC 434.
V0625 Ori |In the region of T-association FU Ori.
V0626 Ori |In the region of T-association FU Ori.
V0627 Ori |In the region of T-association FU Ori.
V0628 Ori |In the region of T-association FU Ori.
V0629 Ori |In the region of T-association FU Ori.
V0630 Ori |In the region of T-association FU Ori.
V0631 Ori |In the region of T-association FU Ori.
V0632 Ori |In the region of T-association FU Ori.
V0634 Ori |In the region of T-association FU Ori.
V0635 Ori |In the region of T-association FU Ori.
V0636 Ori |In the region of T-association FU Ori.
V0637 Ori |In the region of T-association FU Ori.
V0638 Ori |In the region of T-association FU Ori.
V0639 Ori |In the region of T-association FU Ori.
V0640 Ori |d <= 0.02P.
V0641 Ori |Min II 14.5.
V0642 Ori |d = 0.05P?.
V0643 Ori |P = 26.2075d?
V0647 Ori |Min II 11.9. P var. Min I = 2418005.035 + 0.977575d*E
V0647 Ori |(JD2414660 - 23230); since JD2423230 - see Table.
V0648 Ori |Min II 12.2.
V0649 Ori |In the T-association CO - Ori. VB A (B 15m, 2", 0deg).
V0650 Ori |In the region of the open cluster lambda Ori.
V0652 Ori |In the region of the Orion nebula T-association.
V0654 Ori |In the region of the Orion nebula T-association.
V0655 Ori |In the region of the Orion nebula T-association.
V0656 Ori |In the region of the Orion nebula T-association.
V0657 Ori |In the region of the Orion nebula T-association.
V0658 Ori |In the region of the Orion nebula T-association.
V0659 Ori |In the region of the Orion nebula T-association.
V0667 Ori |Min II 15.0.
V0676 Ori |In the region of the Orion nebula T-association.
V0677 Ori |In the region of the Orion nebula T-association.
V0678 Ori |In the region of the Orion nebula T-association.
V0679 Ori |In the region of the Orion nebula T-association.
V0680 Ori |In the region of the Orion nebula T-association.
V0681 Ori |In the region of the Orion nebula T-association.
V0682 Ori |In the region of the Orion nebula T-association.
V0683 Ori |In the region of the Orion nebula T-association.
V0684 Ori |In the region of the Orion nebula T-association.
V0685 Ori |In the region of the Orion nebula T-association.
V0685 Ori |A(U) = 1.0m.
V0686 Ori |In the region of the Orion nebula T-association.
V0687 Ori |In the region of the Orion nebula T-association.
V0688 Ori |In the region of the Orion nebula T-association.
V0689 Ori |In the region of the Orion nebula T-association.
V0690 Ori |In the region of the Orion nebula T-association.
V0691 Ori |In the region of the Orion nebula T-association.
V0692 Ori |In the region of the Orion nebula T-association.
V0693 Ori |In the region of the Orion nebula T-association.
V0694 Ori |In the region of the Orion nebula T-association.
V0695 Ori |In the region of the Orion nebula T-association.
V0696 Ori |In the region of the Orion nebula T-association.
V0697 Ori |In the region of the Orion nebula T-association.
V0698 Ori |In the region of the Orion nebula T-association.
V0699 Ori |In the region of the Orion nebula T-association.
V0700 Ori |In the region of the Orion nebula T-association.
V0701 Ori |In the region of the Orion nebula T-association.
V0702 Ori |In the region of the Orion nebula T-association.
V0703 Ori |In the region of the Orion nebula T-association.
V0704 Ori |In the region of the Orion nebula T-association.
V0705 Ori |In the region of the Orion nebula T-association.
V0706 Ori |In the region of the Orion nebula T-association.
V0707 Ori |In the region of the Orion nebula T-association.
V0708 Ori |In the region of the Orion nebula T-association.
V0709 Ori |In the region of the Orion nebula T-association.
V0710 Ori |In the region of the Orion nebula T-association.
V0711 Ori |In the region of the Orion nebula T-association.
V0712 Ori |In the region of the Orion nebula T-association.
V0713 Ori |In the region of the Orion nebula T-association.
V0713 Ori |A(U) = 4.0m.
V0714 Ori |In the region of the Orion nebula T-association.
V0715 Ori |In the region of the Orion nebula T-association.
V0716 Ori |In the region of the Orion nebula T-association.
V0717 Ori |In the region of the Orion nebula T-association.
V0718 Ori |In the region of the Orion nebula T-association.
V0718 Ori |Probably the sf-component of a very close pair.
V0719 Ori |In the region of the Orion nebula T-association.
V0720 Ori |In the region of the Orion nebula T-association.
V0721 Ori |In the region of the Orion nebula T-association.
V0722 Ori |In the region of the Orion nebula T-association.
V0723 Ori |In the region of the Orion nebula T-association.
V0724 Ori |In the region of the Orion nebula T-association.
V0725 Ori |In the region of the Orion nebula T-association.
V0726 Ori |In the region of the Orion nebula T-association.
V0727 Ori |In the region of the Orion nebula T-association.
V0728 Ori |In the region of the Orion nebula T-association.
V0729 Ori |In the region of the Orion nebula T-association.
V0730 Ori |In the region of the Orion nebula T-association.
V0731 Ori |In the region of the Orion nebula T-association.
V0732 Ori |In the region of the Orion nebula T-association.
V0733 Ori |In the region of the Orion nebula T-association.
V0734 Ori |In the region of the Orion nebula T-association.
V0735 Ori |In the region of the Orion nebula T-association.
V0736 Ori |In the region of the Orion nebula T-association.
V0737 Ori |In the region of the Orion nebula T-association.
V0737 Ori |A(U) > 2.4m.
V0738 Ori |In the region of the Orion nebula T-association.
V0739 Ori |In the region of the Orion nebula T-association.
V0740 Ori |In the region of the Orion nebula T-association.
V0740 Ori |A(pg) > 4.0m.
V0741 Ori |In the region of the Orion nebula T-association.
V0742 Ori |In the region of the Orion nebula T-association.
V0744 Ori |In the region of the Orion nebula T-association.
V0745 Ori |In the region of the Orion nebula T-association.
V0746 Ori |In the region of the Orion nebula T-association.
V0747 Ori |In the region of the Orion nebula T-association.
V0748 Ori |In the region of the Orion nebula T-association.
V0749 Ori |In the region of the Orion nebula T-association.
V0750 Ori |In the region of the Orion nebula T-association.
V0751 Ori |In the region of the Orion nebula T-association.
V0752 Ori |In the region of the Orion nebula T-association.
V0753 Ori |In the region of the Orion nebula T-association.
V0754 Ori |In the region of the Orion nebula T-association.
V0755 Ori |In the region of the Orion nebula T-association.
V0756 Ori |In the region of the Orion nebula T-association.
V0757 Ori |In the region of the Orion nebula T-association.
V0758 Ori |In the region of the Orion nebula T-association.
V0759 Ori |In the region of the Orion nebula T-association.
V0760 Ori |In the region of the Orion nebula T-association.
V0761 Ori |In the region of the Orion nebula T-association.
V0762 Ori |In the region of the Orion nebula T-association.
V0763 Ori |In the region of the Orion nebula T-association.
V0764 Ori |In the region of the Orion nebula T-association.
V0765 Ori |In the region of the Orion nebula T-association.
V0766 Ori |In the region of the Orion nebula T-association.
V0767 Ori |In the region of the Orion nebula T-association.
V0767 Ori |A(U) = 1.5m.
V0768 Ori |In the region of the Orion nebula T-association.
V0770 Ori |In the region of the Orion nebula T-association.
V0771 Ori |In the region of the Orion nebula T-association.
V0772 Ori |In the region of the Orion nebula T-association.
V0773 Ori |In the region of the Orion nebula T-association.
V0774 Ori |In the region of the Orion nebula T-association.
V0775 Ori |In the region of the Orion nebula T-association.
V0776 Ori |In the region of the Orion nebula T-association.
V0777 Ori |In the region of the Orion nebula T-association.
V0778 Ori |In the region of the Orion nebula T-association.
V0778 Ori |A(pg) = 1.6m.
V0779 Ori |In the region of the Orion nebula T-association.
V0780 Ori |In the region of the Orion nebula T-association.
V0780 Ori |A(U) = 1.0m.
V0781 Ori |In the region of the Orion nebula T-association.
V0782 Ori |In the region of the Orion nebula T-association.
V0783 Ori |In the region of the Orion nebula T-association.
V0783 Ori |A(pg) = 3.0m.
V0784 Ori |In the region of the Orion nebula T-association.
V0785 Ori |In the region of the Orion nebula T-association.
V0786 Ori |In the region of the Orion nebula T-association.
V0787 Ori |In the region of the Orion nebula T-association.
V0788 Ori |In the region of the Orion nebula T-association.
V0789 Ori |In the region of the Orion nebula T-association.
V0790 Ori |In the region of the Orion nebula T-association.
V0791 Ori |In the region of the Orion nebula T-association.
V0792 Ori |In the region of the Orion nebula T-association.
V0793 Ori |In the region of the Orion nebula T-association.
V0794 Ori |In the region of the Orion nebula T-association.
V0795 Ori |In the region of the Orion nebula T-association.
V0796 Ori |In the region of the Orion nebula T-association.
V0797 Ori |In the region of the Orion nebula T-association.
V0798 Ori |In the region of the Orion nebula T-association.
V0799 Ori |In the region of the Orion nebula T-association.
V0800 Ori |In the region of the Orion nebula T-association.
V0801 Ori |In the region of the Orion nebula T-association.
V0802 Ori |In the region of the Orion nebula T-association.
V0803 Ori |In the region of the Orion nebula T-association.
V0804 Ori |In the region of the Orion nebula T-association.
V0805 Ori |In the region of the Orion nebula T-association.
V0806 Ori |In the region of the Orion nebula T-association.
V0807 Ori |In the region of the Orion nebula T-association.
V0808 Ori |In the region of the Orion nebula T-association.
V0810 Ori |In the region of the Orion nebula T-association.
V0811 Ori |In the region of the Orion nebula T-association.
V0812 Ori |In the region of the Orion nebula T-association.
V0813 Ori |In the region of the Orion nebula T-association.
V0814 Ori |In the region of the Orion nebula T-association.
V0815 Ori |In the region of the Orion nebula T-association.
V0816 Ori |In the region of the Orion nebula T-association.
V0817 Ori |In the region of the Orion nebula T-association.
V0818 Ori |In the region of the Orion nebula T-association.
V0819 Ori |In the region of the Orion nebula T-association.
V0820 Ori |In the region of the Orion nebula T-association.
V0821 Ori |In the region of the Orion nebula T-association.
V0822 Ori |In the region of the Orion nebula T-association.
V0823 Ori |In the region of the Orion nebula T-association.
V0824 Ori |In the region of the Orion nebula T-association.
V0825 Ori |In the region of the Orion nebula T-association.
V0826 Ori |In the region of the Orion nebula T-association.
V0827 Ori |In the region of the Orion nebula T-association.
V0828 Ori |In the region of the Orion nebula T-association.
V0829 Ori |In the region of the Orion nebula T-association.
V0830 Ori |In the region of the Orion nebula T-association.
V0831 Ori |In the region of the Orion nebula T-association.
V0832 Ori |In the region of the Orion nebula T-association.
V0833 Ori |In the region of the Orion nebula T-association.
V0834 Ori |In the region of the Orion nebula T-association.
V0835 Ori |In the region of the Orion nebula T-association.
V0836 Ori |In the region of the Orion nebula T-association.
V0836 Ori |A(U) > 1.5m.
V0837 Ori |In the region of the Orion nebula T-association.
V0838 Ori |In the region of tbe Orion nebula T-association.
V0839 Ori |In the region of tbe Orion nebula T-association.
V0840 Ori |In the region of the Orion nebula T-association.
V0840 Ori |A(pg) = 0.7m.
V0841 Ori |In the region of the Orion nebula T-association.
V0842 Ori |In the region of the Orion nebula T-association.
V0843 Ori |In the region of the Orion nebula T-association.
V0844 Ori |In the region of the Orion nebula T-association.
V0845 Ori |In the region of the Orion nebula T-association.
V0846 Ori |In the region of the Orion nebula T-association.
V0847 Ori |In the region of the Orion nebula T-association.
V0848 Ori |In the region of the Orion nebula T-association.
V0849 Ori |In the region of the Orion nebula T-association.
V0850 Ori |In the region of the Orion nebula T-association.
V0851 Ori |In the region of the Orion nebula T-association.
V0852 Ori |In the region of the Orion nebula T-association.
V0853 Ori |In the region of the Orion nebula T-association.
V0854 Ori |In the region of the Orion nebula T-association.
V0855 Ori |In the region of the Orion nebula T-association.
V0855 Ori |A(U) > 2.0m.
V0856 Ori |In the region of the Orion nebula T-association.
V0857 Ori |In the region of the Orion nebula T-association.
V0857 Ori |A(pg) > 5.0m.
V0858 Ori |In the region of the Orion nebula T-association.
V0859 Ori |In the region of the Orion nebula T-association.
V0860 Ori |In the region of the Orion nebula T-association.
V0861 Ori |In the region of the Orion nebula T-association.
V0862 Ori |In the region of the Orion nebula T-association.
V0863 Ori |In the region of the Orion nebula T-association.
V0864 Ori |In the region of the Orion nebula T-association.
V0865 Ori |In the region of the Orion nebula T-association.
V0866 Ori |In the region of the Orion nebula T-association.
V0867 Ori |In the region of the Orion nebula T-association.
V0867 Ori |A(pg)>3.0m.
V0868 Ori |In the region of the Orion nebula T-association.
V0869 Ori |In the region of the Orion nebula T-association.
V0870 Ori |In the region of the Orion nebula T-association.
V0871 Ori |In the region of the Orion nebula T-association.
V0872 Ori |In the region of the Orion nebula T-association.
V0873 Ori |In the region of the Orion nebula T-association.
V0874 Ori |In the region of the Orion nebula T-association.
V0875 Ori |In the region of the Orion nebula T-association.
V0876 Ori |In the region of the Orion nebula T-association.
V0876 Ori |Southem component of a close pair.
V0877 Ori |In the region of the Orion nebula T-association.
V0878 Ori |In the region of the Orion nebula T-association.
V0879 Ori |In the region of the Orion nebula T-association.
V0880 Ori |In the region of the Orion nebula T-association.
V0881 Ori |In the region of the Orion nebula T-association.
V0882 Ori |In the region of the Orion nebula T-association.
V0883 Ori |In the region of the Orion nebula T-association.
V0883 Ori |In the apex of a cometary nebula.
V0884 Ori |In the region of the Orion nebula T-association.
V0885 Ori |In the region of the Orion nebula T-association.
V0886 Ori |In the region of the Orion nebula T-association.
V0886 Ori |A(pg) > 3.5m.
V0888 Ori |In the region of the Orion nebula T-association.
V0889 Ori |In the region of the Orion nebula T-association.
V0890 Ori |In the region of the Orion nebula T-association.
V0891 Ori |In the region of the Orion nebula T-association.
V0892 Ori |In the region of the Orion nebula T-association.
V0892 Ori |Southern component of a pair (ro = 3").
V0893 Ori |In the region of the Orion nebula T-association.
V0893 Ori |A(U) = 2.0m.
V0894 Ori |In the region of the Orion nebula T-association.
V0895 Ori |In the region of the Orion nebula T-association.
V0896 Ori |In the region of the Orion nebula T-association.
V0897 Ori |In the region of the Orion nebula T-association.
V0898 Ori |In the region of the Orion nebula T-association.
V0899 Ori |In the region of the Orion nebula T-association.
V0900 Ori |In the region of the Orion nebula T-association.
V0900 Ori |A(pg) > 2.5m.
V0901 Ori |In the region of the nebula IC 434.
V0902 Ori |In the region of the Orion nebula T-association.
V0904 Ori |In the region of the Orion nebula T-association.
V0905 Ori |In the region of the Orion nebula T-association.
V0906 Ori |In the region of the Orion nebula T-association.
V0907 Ori |In the region of the Orion nebula T-association.
V0908 Ori |In the region of the Orion nebula T-association.
V0909 Ori |In the region of the Orion nebula T-association.
V0916 Ori |P = 0.28297d? Member of the open cluster NGC 2169.
V0917 Ori |Member of the open cluster NGC 2169.
V0918 Ori |In the region of the Orion nebula T-association.
V0919 Ori |In the region of the Orion nebula T-association.
V0920 Ori |In the region of the Orion nebula T-association.
V0921 Ori |In the region of the Orion nebula T-association.
V0922 Ori |In the region of the Orion nebula T-association.
V0923 Ori |In the region of the Orion nebula T-association.
V0924 Ori |In the region of the Orion nebula T-association.
V0926 Ori |In the region of the Orion nebula T-association.
V0927 Ori |In the region of the Orion nebula T-association.
V0928 Ori |In the region of the Orion nebula T-association.
V0929 Ori |In the region of the Orion nebula T-association.
V0930 Ori |In the region of the Orion nebula T-association.
V0931 Ori |In the region of the Orion nebula T-association.
V0932 Ori |In the region of the Orion nebula T-association.
V0933 Ori |In the region of the Orion nebula T-association.
V0934 Ori |In the region of the Orion nebula T-association.
V0935 Ori |In the region of the Orion nebula T-association.
V0937 Ori |In the region of the Orion nebula T-association.
V0938 Ori |In the region of the Orion nebula T-association.
V0939 Ori |In the region of the Orion nebula T-association.
V0941 Ori |In the region of the Orion nebula T-association.
V0942 Ori |In the region of the Orion nebula T-association.
V0943 Ori |In the region of the Orion nebula T-association.
V0945 Ori |In the region of the Orion nebula T-association.
V0946 Ori |In the region of the Orion nebula T-association.
V0947 Ori |In the region of the Orion nebula T-association.
V0948 Ori |In the region of the Orion nebula T-association.
V0949 Ori |In the region of the Orion nebula T-association.
V0950 Ori |In the region of the Orion nebula T-association.
V0951 Ori |In the region of the Orion nebula T-association.
V0952 Ori |In the region of the Orion nebula T-association.
V0953 Ori |In the region of the nebula IC 434.
V0956 Ori |In the region of the nebula IC 434.
V0957 Ori |In the region of the nebula IC 434.
V0958 Ori |In the region of the Orion nebula T-association.
V0960 Ori |In the region of the nebula IC 434.
V0961 Ori |In the region of the Orion nebula T-association.
V0964 Ori |P var. Max = 2415800.389 + 0.5046772d*E
V0964 Ori |(JD2415800 - 21010); Max = 2424500.446 + 0.50466477d*E
V0964 Ori |(JD2424500 - 30500); since JD2431500 - see Table.
V0966 Ori |In the region of the Orion nebula T-association.
V0967 Ori |In the region of the Orion nebula T-association.
V0968 Ori |In the region of the Orion nebula T-association.
V0969 Ori |In the region of the Orion nebula T-association.
V0970 Ori |In the region of the Orion nebula T-association.
V0971 Ori |In the region of the Orion nebula T-association.
V0972 Ori |In the region of the Orion nebula T-association.
V0973 Ori |In the region of the Orion nebula T-association.
V0974 Ori |In the region of the Orion nebula T-association.
V0975 Ori |In the region of the Orion nebula T-association.
V0976 Ori |In the region of the Orion nebula T-association.
V0977 Ori |In the region of the Orion nebula T-association.
V0978 Ori |In the region of the Orion nebula T-association.
V0979 Ori |In the region of the Orion nebula T-association.
V0980 Ori |In the region of the Orion nebula T-association.
V0981 Ori |In the region of the Orion nebula T-association.
V0982 Ori |In the region of the Orion nebula T-association.
V0983 Ori |In the region of the Orion nebula T-association.
V0984 Ori |In the region of the Orion nebula T-association.
V0985 Ori |In the region of the Orion nebula T-association.
V0986 Ori |In the region of the Orion nebula T-association.
V0987 Ori |In the region of the Orion nebula T-association.
V0988 Ori |In the region of the Orion nebula T-association.
V0989 Ori |In the region of the Orion nebula T-association.
V0990 Ori |In the region of the Orion nebula T-association.
V0991 Ori |In the region of the Orion nebula T-association.
V0992 Ori |In the region of the Orion nebula T-association.
V0994 Ori |In the region of the Orion nebula T-association.
V0995 Ori |In the region of the Orion nebula T-association.
V0996 Ori |In the region of the Orion nebula T-association.
V0997 Ori |In the region of the Orion nebula T-association.
V0998 Ori |mu = 0.28", ro = 221deg.
V0999 Ori |In the region of the Orion nebula T-association.
V1000 Ori |In the region of the Orion nebula T-association.
V1001 Ori |In the region of the Orion nebula T-association.
V1002 Ori |In the region of the Orion nebula T-association.
V1003 Ori |mu = 0.272", ro = 60.8deg.
V1004 Ori |VB A (B 10.57m, 37", 204deg); SB (P = 2.74d).
V1005 Ori |The range of light variations (characteristic for BY Dra
V1005 Ori |type variability) between the flares is given in the Table;
V1005 Ori |the amplitude of the flares A(U) can reach 3.2m.
V1006 Ori |In the region of the Orion nebula T-association.
V1007 Ori |In the region of the Orion nebula T-association.
V1016 Ori |In the region of the Orion nebula T-association.
V1016 Ori |In the cluster NGC 1976. Orion Trapezium
V1016 Ori |member: teta1 Ori A (B = BM Ori, 8.7", 32deg; C 5.13m,
V1016 Ori |13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.001P.
V1017 Ori |In the region of the Orion nebula T-association.
V1018 Ori |In the region of the Orion nebula T-association.
V1019 Ori |In the region of the Orion nebula T-association.
V1020 Ori |In the region of the Orion nebula T-association.
V1022 Ori |In the region of T-association FU Ori.
V1028 Ori |P = 6d?
V1029 Ori |In the region of the Orion nebula T-association.
V1030 Ori |In the region of the nebula IC 434. (sig Ori) E
V1030 Ori |(A 4.1m; B 5.1m, A = 0.247", P = 170yr; C 8.79m, 11.2",
V1030 Ori |238deg; D 6.66m, 12.9", 84deg; E 41.6", 61deg). Min I
V1030 Ori |(HeI) = 2442802.48 + 1.19080d*E. Unusual helium variable.
V1030 Ori |Epoch of Min I brightness is given in the Table
V1030 Ori |(Min II 6.71, Min II - Min I = 0.43P). This epoch is being
V1030 Ori |observed by 0.18P later than the epoch of minimum strength
V1030 Ori |of the HeI lambda 4026 A line. According to [09524], light
V1030 Ori |minima are due to "eclipses" of the star surface
V1030 Ori |by two isolated clouds (consisting of hydrogen and
V1030 Ori |helium), which are located almost oppositely near
V1030 Ori |the intersections of the magnetic And rotational
V1030 Ori |equator.
V1031 Ori |VB (0.159", 104deg, 1980.7). Min II 6.32; DII = 0.017P.
V1034 Ori |Epoch of light minimum is given.
V1035 Ori |In the region of the Orion nebula T-association.
V1036 Ori |In the region of the Orion nebula T-association.
V1037 Ori |In the region of the Orion nebula T-association.
V1038 Ori |In the region of the Orion nebula T-association.
V1039 Ori |In the region of the Orion nebula T-association.
V1040 Ori |In the region of the Orion nebula T-association.
V1041 Ori |In the region of the Orion nebula T-association.
V1042 Ori |In the region of the Orion nebula T-association.
V1043 Ori |In the region of the Orion nebula T-association.
V1044 Ori |In the region of the Orion nebula T-association.
V1045 Ori |In the region of the Orion nebula T-association.
V1046 Ori |In the region of the Orion nebula T-association.
V1046 Ori |SB 1. Min II 6.58. Possibly an ellipsoidal variable, its
V1046 Ori |light variations being superimposed by light variations of
V1046 Ori |the primary component of SX Ari type:
V1046 Ori |Min (HeI) = 2442812.23 + 0.9015d*E [08054].
V1047 Ori |In the region of the Orion nebula T-association.
V1048 Ori |In the region of the Orion nebula T-association.
V1049 Ori |In the region of the Orion nebula T-association.
V1050 Ori |In the region of the Orion nebula T-association.
V1052 Ori |In the region of the Orion nebula T-association.
V1053 Ori |In the region of the Orion nebula T-association.
V1054 Ori |Epoch of light minimum is given. P = 8.596d?, P = 8.674d?
V1055 Ori |P(X) = 5.2d [09528].
V1056 Ori |VB A (B 9.8m, 28.7", 58deg).
V1058 Ori |In the region of the Orion nebula T-association.
V1059 Ori |In the region of the Orion nebula T-association.
V1060 Ori |In the region of the Orion nebula T-association.
V1061 Ori |In the region of the Orion nebula T-association.
V1062 Ori |In the region of the Orion nebula T-association.
V1063 Ori |In the region of the Orion nebula T-association.
V1064 Ori |In the region of the Orion nebula T-association.
V1065 Ori |In the region of the Orion nebula T-association.
V1066 Ori |In the region of the Orion nebula T-association.
V1067 Ori |In the region of the Orion nebula T-association.
V1068 Ori |In the region of the Orion nebula T-association.
V1069 Ori |In the region of the Orion nebula T-association.
V1070 Ori |In the region of the Orion nebula T-association.
V1071 Ori |In the region of the Orion nebula T-association.
V1072 Ori |In the region of the Orion nebula T-association.
V1073 Ori |In the region of the Orion nebula T-association.
V1074 Ori |In the region of the Orion nebula T-association.
V1075 Ori |In the region of the Orion nebula T-association.
V1076 Ori |In the region of the Orion nebula T-association.
V1077 Ori |In the region of the Orion nebula T-association.
V1078 Ori |In the region of the Orion nebula T-association.
V1079 Ori |In the region of the Orion nebula T-association.
V1080 Ori |In the region of the Orion nebula T-association.
V1081 Ori |In the region of the Orion nebula T-association.
V1082 Ori |In the region of the Orion nebula T-association.
V1083 Ori |In the region of the Orion nebula T-association.
V1084 Ori |In the region of the Orion nebula T-association.
V1377 Ori |SB?, Porb ~ 5.5 to 6.5d.
V1380 Ori |In a bright nebula.
alf   Ori |VB A (B 14.5m, 39.8", 110deg). Min = 2410600 + 2070d*E
alf   Ori |(1840 - 1929) [01012]. Since 1929 - see Table.
alf   Ori |The main variation is superimposed by the waves
alf   Ori |with P = 200 - 400d. Dust-gaseous shell (r = 50")
alf   Ori |[09529].
del   Ori |VB A (A 0.217", 144deg, 1980; B 14.0m, 33.1", 227deg;
del   Ori |C 6.84m, 53.5", 359deg). Orion Belt cluster member.
del   Ori |Min II 2.20.
del   Ori |Apsidal motion (P = 210 yr). Shape of the light curve
del   Ori |varies. The intrinsic brightness variability of the
del   Ori |components is possible.
eps   Ori |Orion Belt cluster member.
eta   Ori |VB Aab (AC 0.037", 111deg, 1979.0, P = 9.219 yr [09535];
eta   Ori |B 4.8m, 1.60", 76deg, 1976.0; C 9.4m, 115", 51deg). EA/DM.
eta   Ori |Min II 3.57. The range of combined light variation of the
eta   Ori |components AAb (SB 2, P = 7.989268d), AC, and B is given
eta   Ori |in the Table. Outside eclipses there are sinusoidal light
eta   Ori |variations of the system with A(V) = 0.05m due to
eta   Ori |pulsations of the component Ab [09535] with P = 0.30197d
eta   Ori |[09536] or 0.30145d [09537]. According to [08566] these
eta   Ori |variations were not observed between 1970 and 1976.
pi  5 Ori |Min II 3.73. The period is improved using radial
pi  5 Ori |velocities [04627].
psi   Ori |VB A (B 11.1m, 2.7", 323deg; C 13.88m, 83", 196deg).
psi   Ori |Min II 4.58. The period is determined on the base of
psi   Ori |radial velocities [09541].
R     Pav |Pvar. Max = 2411219 + 228.34d (JD2411000 - 18500);
R     Pav |Max = 2418527 + 230.95d*E (JD2418500 - 30000);
R     Pav |since JD2430000 - see Table.
S     Pav |P var. Max = 2421479 + 389.64d*E(JD2421000 - 31000);
S     Pav |since JD2431000 - see Table. Delta(m) var strongly.
S     Pav |Min II is sometimes observed after Max I.
T     Pav |P var. Max = 2413328 + 243.45d*E(JD2405700 -
T     Pav |25500); Max = 2425499 + 245.11d*E(JD2425500 -
T     Pav |32500); since JD2432500 - see Table.
V     Pav |VBA (B 14.0m vis, 15", 327deg). Mean brightness var,
V     Pav |P2 = 3735d, 9.7m - 10.7m.
W     Pav |P var. Before JD2431000 Max = 2413778 + 282.92d*E;
W     Pav |since JD2431000 - see Table.
RT    Pav |Mean light var, 10.4m - 11.1m  1649, P2 = 757d.
SU    Pav |P var. Max = 2430036 + 245.18d*E (JD2411000 - 30100)
SU    Pav |[00001]; during JD247700 - 40000 - see Table.
SX    Pav |mu alpha = +0.0166s, mu delta = -0.05".
TW    Pav |Before JD2420400 Max = 2417760 + 397.d*E.
YY    Pav |Delta(m) var strongly. P possibly is twice longer, in that
YY    Pav |case Min II 14.4.
AR    Pav |Depth of eclipses Delta(m) = 2m B, d = 0.05P. Expanding
AR    Pav |shell.
BD    Pav |Only one outburst was observed [00629]. Brightness
BD    Pav |flickering. Eclipses according to the elements
BD    Pav |Min I = 2444412.676 + 0.1793015d*E, Delta(m) ~0.5m [09191].
BD    Pav |Outside outburst, 15.40m - 16.21m.
BF    Pav |Min II 11.9.
BI    Pav |Min II (Delta(m) ~0.05m) is possible.
DF    Pav |Epoch of min is given. Light curve shape strongly var.
DN    Pav |Delta(S) = 8:.
DW    Pav |Min II 16.3.
EG    Pav |Twice shorter P is possible [00001].
EL    Pav |Min II 15.5.
EN    Pav |Elements need confirmation.
EQ    Pav |Red.
FY    Pav |Min II? JD2436784.37.
HL    Pav |Blazhko effect?
HP    Pav |Min II 15.5.
HQ    Pav |Min II 12.7.
HY    Pav |Min II 12.1.
IL    Pav |RRC type is possible.
KR    Pav |Min II 14.1.
KZ    Pav |VB A (B 8.7m, 6.7", 119deg, 1971; C 9.2m, BC 1.0", 329deg,
KZ    Pav |1971). P var. Min = 2430448.617 + 0.949880d*E
KZ    Pav |(JD2416000 - 30000) [00001]; since JD2430000 - see Table.
KZ    Pav |Min II is present.
LL    Pav |Min II 15.1.
LO    Pav |Min II 16.5.
LR    Pav |Min II 15.3.
LT    Pav |Min II 12.2.
LV    Pav |Min II 14.3.
LY    Pav |Min II 14.9.
MQ    Pav |Epoch of Min is given. EW/KW type with twice longer P is
MQ    Pav |possible.
MR    Pav |Possible elements Max = 2436731.40 + 0.3737d*E [00001].
MS    Pav |Min II 14.1.
MW    Pav |d = 0.08P. Min II 8.92, dII = 0.11P.
NP    Pav |Deep Min II.
NW    Pav |[A/H] = -0.7.
OY    Pav |The chart in [06286] is wrong.
V0382 Pav |Type EW: is also possible.
kap   Pav |P var. Max = 2419619.38 + 9.0898d*E (JD2411930 - 22550);
kap   Pav |Max = 2425987.12 + 9.1028d*E (JD2422550 - 26980);
kap   Pav |Max = 2430530.67 + 9.0833d*E (JD2426980 - 31345);
kap   Pav |Max = 2433239.87 + 9.0956d*E (JD2431345 - 34045);
kap   Pav |Max = 2434693.11 + 9.0653d*E (JD2434045 - 37000);
kap   Pav |since JD2440000 - see Table. [Fe/H] = 0.0/ - 0.4.
kap   Pav |Moderately high Z coordinate (IZI ~240 pc provided
kap   Pav |the period - luminosity relation for DCEP stars is valid),
kap   Pav |low radial velocity. The period is not typical
kap   Pav |for CW stars. Ca II emission was noticed in the spectrum.
lam   Pav |VB A (B 12.4m, 63.1", 206deg).
rho   Pav |The main light variation P1 (see Table) with a
rho   Pav |semiamplitude delta(y) = 0.0069m is superposed by
rho   Pav |oscillations with P2 = 0.1131d (delta(y) = 0.0031m),
rho   Pav |P3 = 0.1612d (delta(y) = 0.0029m).
R     Peg |OH, H2O, SiO maser. P var. Max = 2396327 + 381.9d*E
R     Peg |(JD2396300 - 2408200); Max = 2413012 + 371.4d*E
R     Peg |(JD2413000 - 19800); Max = 2420092 + 379.77d*E
R     Peg |(JD2420000 - 31100) [00960]; since JD2431100 - see Table.
T     Peg |P var. Max = 2398452 + 371.0d*E (JD2398400 - 2408900);
T     Peg |Max = 2413697 + 386.8d*E (JD2413600 - 18700);
T     Peg |Max = 2421016 + 362.5d*E (JD2420900 - 28000) [00960];
T     Peg |Max = 2434343 + 376.0d*E (JD2428300 - 34300);
T     Peg |Max = 2440984 + 368.7d*E (JD2434300 - 41000);
T     Peg |since JD2441000 - see Table.
U     Peg |Min II 9.73. P var.
U     Peg |There is a square term in the elements:
U     Peg |-2.468D*10**(-11)*E**2.
U     Peg |0 - C = 0.00323d*sin((2pi/16330)E + 0.418pi). Shape of
U     Peg |the light curve varies.
W     Peg |SiO maser. P var. Max = 2413819 + 343.2d*E
W     Peg |(JD2413800 - 26600); Max = 2427162 + 345.5d*E
W     Peg |(JD2426600 - 32100) [00960]; Max = 2439690 + 348.75d*E
W     Peg |(JD2432300 - 39700) [00001]; since JD2441400 - see Table.
X     Peg |P var. Max = 2414713 + 200.3d*E (JD2414700 - 21300);
X     Peg |Max = 2420105 + 204.3d*E (JD2420100 - 23800);
X     Peg |Max = 2423570 + 199.8d*E (JD2423600 - 31000) [00960];
X     Peg |Max = 2432006 + 208d*E (JD2431000 - 32100);
X     Peg |Max = 2434206 + 200.0d*E (JD2432100 - 39300);
X     Peg |since JD2438400 - see Table.
Z     Peg |P var. Max = 2415433 + 318.9d*E (JD2398800 - 2420550);
Z     Peg |Max = 2420207 + 328.0d*E (JD2420200 - 32000) [00960];
Z     Peg |Max = 2432005 + 325.8d*E (JD2432000 - 37900);
Z     Peg |Max = 2437870 + 319d*E (JD2437500 - 40100);
Z     Peg |Max = 2442086 + 328.0d*E (JD2440100 - 43100);
Z     Peg |since JD2442100 - see Table.
RR    Peg |P var. Max = 2417582 + 268.3d*E (JD2416700 - 17850)
RR    Peg |[00001]; Max = 2417859 + 260.8d*E (JD2417850 - 21000)
RR    Peg |[00960]; since JD2421000 - see Table.
RS    Peg |P var. Max = 2415846 + 431.5d*E (JD2415800 - 18450);
RS    Peg |Max = 2418434 + 404.1d*E (JD2418400 - 24200);
RS    Peg |Max = 2424514 + 413.4d*E (JD2424500 - 34900) [00960];
RS    Peg |Max = 2436496 + 403.4d*E (JD2435700 - 38600) [00001];
RS    Peg |since JD2438500 - see Table.
RT    Peg |VB A (B 10.5m, 15.6", 291deg). P var.
RT    Peg |Max = 2423609 + 215.0d*E (JD2416000 - 24300);
RT    Peg |Max = 2428149 + 216.6d*E (JD2424300 - 32100);
RT    Peg |since JD2432100 - see Table.
RU    Peg |VB A (B 12.5m, 12", 18deg); SB2 (Porb = 0.3746d [09570]).
RU    Peg |There are also light oscillations with P = 11.6s
RU    Peg |and 50s [09571].
RV    Peg |Emission. Light curve (1907 - 1973) [09572]. P var.
RV    Peg |Max = 2428735 + 388.4d*E (JD2417000 - 32640);
RV    Peg |Max = 2430680 + 390.9d*E (JD2430200 - 38900);
RV    Peg |since JD2438800 - see Table.
RW    Peg |P var. Max = 2419393 + 208.4d*E (JD2412700 - 19400);
RW    Peg |Max = 2421520 + 213.0d*E (JD2419390 - 21550);
RW    Peg |Max = 2427133 + 208.0d*E (JD2421500 - 27150);
RW    Peg |since JD2427300 - see Table.
RX    Peg |P2 = 110d:.
RY    Peg |VB B (A = RZ Peg; B 20", 252deg).
RZ    Peg |VB A (B = RY Peg:20", 252deg). SC 6/9 - e. P var.
RZ    Peg |Max = 2423361 + 441.4d*E (JD2411400 - 26450);
RZ    Peg |Max = 2431215 + 434.0d*E (JD2426400 - 33000);
RZ    Peg |since JD2433000 - see Table.
SS    Peg |P var. Max = 2416390 + 410.8d*E (JD2415500 - 20000);
SS    Peg |Max = 2422235 + 423.8d*E (JD2420000 - 27000);
SS    Peg |Max = 2427270 + 403.4d*E (JD2427000 - 29000);
SS    Peg |Max = 2437218 + 416.35d*E (JD2428500 - 43000);
SS    Peg |since JD2443000 - see Table.
SV    Peg |H2O emission.
SX    Peg |S 2.5/6 e. P var. Max = 2436043 + 306.56d*E
SX    Peg |(JD2414800 - 38300); since JD2438300 - see Table.
TU    Peg |P var. Max = 2417800 + 320.8d*E (JD2404300 - 18450);
TU    Peg |Max = 2420730 + 328.4d*E (JD2418450 - 20800);
TU    Peg |Max = 2428080 + 319.6d*E (JD2420800 - 31600);
TU    Peg |since JD2432800 - see Table.
TW    Peg |H2O maser. The basic light variation with the period given
TW    Peg |in the Table is superimposed by small oscillations
TW    Peg |with P = 94.13d.
TY    Peg |Min II 10.2. P var. Min I hel = 2419520.476 +
TY    Peg |3.0922754d*E (JD2412300 - 19600) [02389]; Min I hel =
TY    Peg |2425918.348 + 3.092252d*E (JD2419600 - 26000)
TY    Peg |[00001]; since JD2426000 - see Table.
TZ    Peg |P var? Max = 2425892 + 213.7d*E (JD2410000 - 28000);
TZ    Peg |since JD2430000 - see Table.
UU    Peg |OH, H2O maser.
UW    Peg |According to [08837] P = 60d.
UX    Peg |P var. Min = 2428428.386 + 1.544618d*E (JD2422100 -
UX    Peg |28430) [00230]; Min = 2431273.597 + 1.544632d*E
UX    Peg |(JD2428420 - 34000) [00001]; since JD2434000 - see Table.
VV    Peg |Delta(S) = 8. P var. Max = 2420105.296 + 0.48837765d*E
VV    Peg |(JD2420000 - 28900); Max = 2433217.268 + 0.48838307d*E
VV    Peg |(JD2432800 - 38000) [03506]; since JD2438000 - see Table.
VW    Peg |P = 2.341295d?
VX    Peg |The basic light variation is superimposed by the secondary
VX    Peg |one with P = 80 - 90d:.
VZ    Peg |[Fe/H] = -1.75.
WW    Peg |P var. Max = 2433142 + 371.6d*E (JD2415670 - 33200)
WW    Peg |[00001]; since JD2436800 - see Table.
ZZ    Peg |Min II 12.5.
AE    Peg |P var. Max = 2415470.866 + 0.4967388d*E (JD2415500 -
AE    Peg |21000); Max = 2426161.544 + 0.496725d*E (JD2425400 -
AE    Peg |31500); Max = 2432632.809 + 0.496692d*E (JD2431500 -
AE    Peg |36000) [00001]; during JD2436000 - 40000 - see Table.
AE    Peg |Delta(S) = 6.3.
AG    Peg |SB2 (Porb = 820d [09580]).
AG    Peg |Maximum of brightness was in 1870, then the very
AG    Peg |slow light decrease was observed that was superimposed
AG    Peg |since 1935 by periodical light oscillations with
AG    Peg |A = 0.4m V
AG    Peg |and P = Porb: Min = 2428250 + 827.d*E ( JD2428000-43000)
AG    Peg |[09587]. After JD2442300 the period probably has changed:
AG    Peg |Min = 2442370 + 760d*E [09587]. In 1962 - 1979 the range of
AG    Peg |brightness was 7.95m - 8.55m V; M - m = 0.50P.
AG    Peg |Light minima correspond to the epochs of inferior
AG    Peg |conjunction of M 3 III component. Spectrum var: Beq
AG    Peg |(1893 - 1919); since 1922 the spectrum is symbiotic one,
AG    Peg |the M star spectrum being more noticeable.
AG    Peg |Surrounded by a radio nebula with 1" half-power diameter.
AN    Peg |P var. Max = 2428045 + 274.1d*E (JD2424500 - 38500)
AN    Peg |[09581]; since JD2438500 - see Table.
AO    Peg |Delta(S) = 4.3.
AQ    Peg |Min II 10.47; d = 0.030P. P var. Min I = 2424749.335 +
AQ    Peg |5.548419d*E (JD2424000 - 34000) [00980];
AQ    Peg |since JD2434000 - see Table.
AS    Peg |Of the two stars circled in the chart in [06286], the southern
AS    Peg |component varies.
AT    Peg |Min II 9.04. P var. Min I = 2425862.337 + 1.1460988d*E
AT    Peg |(JD2425800 - 37500) [00001]; Min I = 2437497.542 +
AT    Peg |1.146080d*E (JD2437490 - 40000) [06101]; Min I =
AT    Peg |2440407*4370 + 1.1461007d*E (JD2440000 - 42400)
AT    Peg |[00001]; since JD2442400 - see Table.
AU    Peg |Cepheid in a close binary system.
AU    Peg |SB1 (Porb = 53.319d, K1 = 41.8 km/s, gamma = -4.1 km/s,
AU    Peg |E = 0.12 [09582]). [Fe/H] = 0.1.
AU    Peg |P var. Max = 2428729.76 + 2.3978d*E (JD2426500 - 28750)
AU    Peg |[00916]; Max = 2433151.976 + 2.38934d*E (JD2433150 - 35800);
AU    Peg |Max = 2439039.08 + 2.39079d*E (JD2435800 - 39100) [00001];
AU    Peg |since JD2441700 - see Table.
AU    Peg |There is a square term in the elements given in the Table:
AU    Peg |+2.246d*10**(-6)*E**2. The shape of the light curve varies:
AU    Peg |0.20P <  M - m < 0.47P.
AV    Peg |P var. Max = 2416347.713 + 0.39036510d*E
AV    Peg |(JD2414000 - 26500) [00752]; Max = 2426582.301 +
AV    Peg |0.39037015d*E (JD2426500 - 36000) [09584];
AV    Peg |since JD2436000 - see Table. [Fe/H] = +0.02.
AW    Peg |d = 0.07P, Min II 7.60.
BB    Peg |Depth of Min II 0.60m.
BB    Peg |There is a square term in the elements given in the Table:
BB    Peg |+2.3d*10**(-11)*E**2. dI = 0.05P; dII = 0.00P.
BF    Peg |P var. Max = 2426589.293 + 0.495796d*E + 2.8d*10**(-9)*E**2
BF    Peg |(JD2426500 - 28800) [00522]; Max = 2433200.312 +
BF    Peg |0.495796d*E (JD2429400 - 33200) [00001]; Max =
BF    Peg |2437583.343 + 0.495674d*E (JD2437500 - 39400)
BF    Peg |[00001]; since JD2442650 - see Table.
BG    Peg |P var. Min = 2427386.3705 + 1.952452d*E (JD2426000 - 35000)
BG    Peg |[03567]; Min = 2436453.509 + 1.95238d*E (JD2435000 - 43500)
BG    Peg |[03624]; since JD2443500 - see Table.
BH    Peg |P var. Max = 2426596.535 + 0.64101381d*E
BH    Peg |(JD2426500 - 28200) [01038]; since JD2434400 - see Table.
BH    Peg |Blazhko effect. A var.
BH    Peg |Max (O - C) = 2442929.03 + 39.8d*N [09588]. (k - b)2 = 0.09;
BH    Peg |Delta(S) = 5.
BI    Peg |Waves with a cycle of 60 - 80d are superimposed.
BK    Peg |Min II 10.47.
BO    Peg |Min II 11.6. P var. Min I = 2427655.460 + 0.5804342d*E
BO    Peg |(JD2426500 - 35100) [02263]; since JD2444000 - see Table.
BP    Peg |P1 = 0.084510d; P1:P0 = 0.77. Beat
BP    Peg |period Pb = 0.3698d [06604].
BU    Peg |Observations are represented by the elements in the
BU    Peg |intervals JD2432000 - 34000, JD2438200 - 41400.
BX    Peg |Depth of Min II 0.62m; dI = 0.05P; dII = 0.00P.
BX    Peg |P var. Min I = 2431323.278 + 0.2804238d*E
BX    Peg |(JD2424700 - 39000) [00279]; since JD2439000 - see Table.
BY    Peg |P var. Min I = 2424745.75 + 0.34193403d*E
BY    Peg |(JD2424700 - 35400); since JD2435000 - see Table.
CC    Peg |Min II 12.9.
CG    Peg |Delta(S) = 2. P var?
CU    Peg |d = 0.010P. P var. Min = 2433895.463 + 3.8801345d*E
CU    Peg |(JD2425500 - 34000) [00001]; Min = 2434221.392 +
CU    Peg |3.880196d*E (JD2434000 - 36500) [07929];
CU    Peg |since JD2436500 - see Table.
CZ    Peg |Min II 13.9.
DF    Peg |Min II 9.2.
DG    Peg |P var. Max = 2425857 + 148.15d*E (JD2425500 -
DG    Peg |33500); since JD2433500 - see Table.
DH    Peg |P var. Max = 2414981.537 + 0.25550478d*E
DH    Peg |(JD2414000 - 24000) [01158];
DH    Peg |Max = 2427695.390 + 0.2555107d*E (JD2424000 - 33500)
DH    Peg |[09590]; since JD2433500 - see Table. [Fe/H] = -0.9.
DI    Peg |Min II 9.59. P var. Min I = 2425644.315 + 0.7118144d*E
DI    Peg |(JD2425500 - 30000) [02431]; Min I = 2437559.4096 +
DI    Peg |0.7118182d*E (JD2430000 - 40000) [09592]; Min I =
DI    Peg |2440159.6796 + 0.71181417d*E (JD2440000 - 44500);
DI    Peg |since JD2444500 - see Table.
DK    Peg |d = 0.04P. P var. Min = 2427745.388 + 1.631801d*E
DK    Peg |(JD2427700 - 33700); since JD2433700 - see Table.
DM    Peg |d = 0.03P; Min II 11.0.
DN    Peg |Mean brightness varies with cycles 800 - 1400d and
DN    Peg |A = 0.2m - 0.4m.
DO    Peg |P var. Min = 2434272.350 + 2.61394d*E (JD2428000 - 34700)
DO    Peg |[00485]; since JD2434700 - see Table.
DV    Peg |Min II 12.1.
DY    Peg |P var. Max = 2432751.9624 + 0.072926372d*E
DY    Peg |(JD2429000 - 38000); since JD2438000 - see Table.
DY    Peg |The basic pulsation is superimposed by the secondary one
DY    Peg |with P1 = 0.05570d [09594]. A var, M - m var (Pi = 0.2358d):
DY    Peg |0.55m < A < 0.67m, 0.24P < M - m < 0.42P. Delta(S) = 6.
DZ    Peg |P var. Max = 2429127.211 + 0.6073407d*E
DZ    Peg |(JD2419000 - 28800); Max = 2429127.189 + 0.6073761d*E
DZ    Peg |(JD2429100 - 33500); since JD2433500 - see Table.
EE    Peg |Min II 7.06. The third body (Porb = 1464d, T0 = 2443120).
EF    Peg |VB B (A 14.0m; B 5", 305deg).
EH    Peg |d = 0.08P.
EQ    PegA|VB A (B = EQb Peg; A = 6.87", Porb = 359 yr, E = 0.20.
EQ    PegA|[09597]); mu = 0.560", P = 91.7deg. A (B) >= 1.4m.
EQ    PegB|VB B (A = EQa Peg). a = 6.87'' P orb = 1464d,
EQ    PegB|T0 = 2443120. A(U) >= 1.9m.
ET    Peg |Delta(S) = 4.
EU    Peg |Min II 12.3.
EZ    Peg |On 1943 November 16 the spectrum of the star was B [02875];
EZ    Peg |probably at that time the star had a flare.
FL    Peg |Min II 14.0.
FU    Peg |Blazhko effect (Pi = 150d); A var;
FU    Peg |15.2m <= Max <= 15.8m; 0.15P <= M - m <= 0.50P.
GH    Peg |Depth of Min II 0.13m.
GR    Peg |P var. Max = 2436492 + 69.93d*E (JD2436420 - 38740);
GR    Peg |since JD2440470 - see Table.
GT    Peg |mu = 0.51", P = 96deg. Epoch of the light minimum is given.
GT    Peg |During the flares A(U) < 3.6m.
GV    Peg |Delta(S) = 5:.
GW    Peg |Min II 15.1.
GX    Peg |SB1 (Porb = 2.340939d [06103]).
GZ    Peg |VB A (B 10.6m, A3V, 32.7", 198deg).
HN    Peg |[Fe/H] = -0.09. Epoch of light minimum is given.
HN    Peg |The variability of emission in H and K call lines with
HN    Peg |P = 4.63d was detected [09600].
HP    Peg |Vr = -381 km/s.
HR    Peg |S4+/1+ .
HZ    Peg |Min II 17.6.
II    Peg |mu = 0.575", p = 86.5deg. SB1
II    Peg |(T0 = 2443030.396 + 6.724464d*E); T0 is the epoch of the
II    Peg |inferior conjunction of K-star. The epoch of the
II    Peg |distortion wave maximum is given in the Table. Mean
II    Peg |brightness of the system varies.
IK    Peg |SB1 (Porb = 21.724d). Multiperiodicity [09609].
IM    Peg |SB1 (Porb = 24.649d).
QQ    Peg |Variability needs confirmation.
V0341 Peg |SB, Porb = 2.1779d.
V0342 Peg |Suspected SB.
bet   Peg |VB A (B 11.2m, 109", 211deg).
eps   Peg |VB A (B 12.66m, 81", 325deg; C 8.65m, 140", 321deg).
eps   Peg |Usually varies in the range 2.29m - 2.44m V. On 1972
eps   Peg |september 26/27 in the interval 23h58m - 00h02m UT it was
eps   Peg |bright (0.7m V), then at 00h09m UT decreased to 2.4m V
eps   Peg |[06875]. On 1847 November 5 the star was 3.5m, then the
eps   Peg |brightness increased but on November 6 it was still
eps   Peg |fainter than normal [09606].
tau   Peg |P2 = 0.04895d; PB = 0.4943d.
S     Per |In the region of the open cluster h, khi Per.
S     Per |OH, H2O, SiO maser.
S     Per |In 1920 - 1969 there were secondary
S     Per |waves with cycles of 300d - 700d and Delta(m) ~1m [08630];
S     Per |in 1935 - 1961 P1 = 807d, P2 = 930d [09694].
T     Per |Other periodicities were noted. In the region
T     Per |of open cluster h, khi Per.
U     Per |P var. Max = 2411683 + 316.10d*E (before JD2422500);
U     Per |Max = 2422748 + 326.53d*E (JD2422500 - 34000);
U     Per |since JD2434000 - see Table.
V     Per |VB A (B 14m, 28", 278deg).
W     Per |P2 = 2667d +- 460d is superimposed.
X     Per |3U 0352 + 30. LX/Lopt = 10**(-2). ADS 2859 A (B =
X     Per |V397 Per, M3III, 22.5", 12deg). SB.
X     Per |IR excess. X-ray pulsar (P = 13.93m).
X     Per |Further periodicities were noticed in X-ray, optical,
X     Per |spectroscopic observations: 22.4h, 308.33d, 580.7d.
Y     Per |P var. Max = 2414990 + 254.74d*E (JD2415000 - 18000);
Y     Per |Max = 2418049 + 246.25d*E (JD2418000 - 22000);
Y     Per |Max = 2422242 + 253.62d*E (JD2422000 - 41000);
Y     Per |since JD2441000 - see Table.
Z     Per |d = 0.028P; Min II 9.8.
Z     Per |P var. Min = 2418173.663 + 3.056422d*E (JD2415000 -
Z     Per |19000) [01961]; Min = 2425481.416 + 3.05636d*E
Z     Per |(JD2419000 - 31000) [00978]; since JD2431000 - see Table.
RR    Per |P var. Max = 2424280 + 392.01d*E (JD2416000 - 28500);
RR    Per |since JD2428500 - see Table.
RS    Per |In the region of the open cluster h, khi Per.
RS    Per |According to [01053], P = 152d.
RT    Per |Min II 10.67. P var. Min = 2411963.2995 + 0.84941322d*E
RT    Per |(JD2411317 - 19400); Min = 2419702.3124 + 0.84940248d*E
RT    Per |(JD2419400 - 29300); Min = 2429751.6066 + 0.84941274d*E
RT    Per |(JD2429300 - 33000); since JD2433000 - see Table.
RV    Per |Min II 10.4. P var. Min = 2417972.345 + 1.973489d*E
RV    Per |(JD2417000 - 25500); since JD2432500 - see Table.
RW    Per |The light curve shape var,
RW    Per |d = 0.03P - 0.000P. Min II 9.78. P var. Before
RW    Per |JD2425720 Min = 2425720.0185 + 13.198910d*E;
RW    Per |Min = 2429217.5946 + 13.198399d*E (JD2425720 - 36700);
RW    Per |since JD2436700 - see Table.
RY    Per |d = 0.014P; Min II 8.65.
RZ    Per |S 3/7 e. P var. Before JD2430500 Max = 2415034 + 353.19d*E;
RZ    Per |since JD2430500 - see Table.
ST    Per |VB A (B 12.1m, 11.6", 6deg, 1928). d = 0.014P, Min II 9.62.
ST    Per |P var. Min = 2419030.5038 + 2.6483615d*E
ST    Per |(JD2418500 - 27000) [09740]; Min = 2429528.5897 +
ST    Per |2.6483488d*E (JD2427000 - 34600) [02389]; Min =
ST    Per |2439091.716 + 2.648353d*E (JD2439000 - 42400);
ST    Per |since JD2442400 - see Table.
SU    Per |In the region of the open cluster h, khi Per.
SV    Per |[A/H] = 0.6. SB2, hot companion.
SV    Per |P var? Before JD2435000 Max = 2419055.145 +
SV    Per |11.12875d*E [02431]; since JD2435000 - see Table.
SX    Per |[A/H] = 0. The chart in [08300]
SY    Per |In the region of the open cluster NGC 1528.
TU    Per |Delta(m), P var. Before JD2427200 Max = 2418572.288 +
TU    Per |0.6070775d*E; Max = 2427119.334 + 0.6070643d*E
TU    Per |(JD2427200 - 36000); since JD2436000 - see Table.
TV    Per |P2 = 1080d is superimposed.
TX    Per |[Fe/H] = -0.88. OH maser.
TZ    Per |VB A (B14m, 13", 290deg). Mu alpha = +0.012",
TZ    Per |mu delta = -0.050". In the region of the open
TZ    Per |cluster h, khi Per.
UX    Per |[A/H] = -0.3.
UY    Per |[A/H] = -0.3. In the region of the open clusters King 4,
UY    Per |Czernik 8.
UZ    Per |P2 = 91d is superimposed.
VV    Per |Twice shorter P is possible [00960].
VX    Per |In the region of the open cluster h, khi Per.
VX    Per |[A/H] = -0.2. P var. Since JD2431000 - see Table.
VY    Per |In the region of the open cluster h, khi Per.
VY    Per |[A/H] = -0.3.
VZ    Per |VB A (B 16.9m pg, 17", 180deg). In the region of the open
VZ    Per |cluster Tr 2.
WY    Per |P var. Min = 2425234.460 + 3.327126d*E (JD2421500 - 26000)
WY    Per |[01072]; since JD2441500 - see Table.
XX    Per |VB A (B 9.7m vis, 21", 176deg, 1909).
XX    Per |Mean brightness var, P = 4100d.
XY    Per |ADS 2788 AB (delta(mV) = 0.6m - 2.5m, 1.4", 75deg,
XY    Per |SpA = A2II, SpB = B6e). IR excess.
XZ    Per |Min II 11.6. P var? Min = 2425150.439 + 1.1516282d*E
XZ    Per |(JD2425000 - 29000) [00522]; Min = 2437932.411 +
XZ    Per |1.1516347d*E + 0.005d*sin(0.09091deg*E) (JD2432000 -
XZ    Per |38000) [00001]; since JD2438000 - see Table.
YZ    Per |In the region of the open cluster h, khi Per.
ZZ    Per |The coordinates are possibly erroneous.
AB    Per |d = 0.045P; Min II 10.5. VB (Delta(m) = 0.0m vis, 0.20",
AB    Per |86.4deg, 1978).
AD    Per |Mean brightness var, P = 2950d.
AD    Per |In the region of the open cluster h, khi Per.
AE    Per |P2 = 2150d is superimposed.
AG    Per |ADS 2990 A (B Delta(m) = 2.0m, 0.9", 225deg, 1975; C 12.6m,
AG    Per |36", 118deg, 1948). The combined brightness AB is given.
AG    Per |Min II 7.00, DII = 0.10P, dII = 0. Apsidal motion:
AG    Per |Min II - Min I = 1.01435d + 0.0884d*sin(0.0278deg*E +
AG    Per |49.1deg).
AR    Per |P var, nonlinear term: +1.18d*10**(-11)*E**2.
AR    Per |[Fe/H] = -0.17.
AS    Per |Delta(m) var, d (Delta(B))/dt = -0.01m/yr.
AV    Per |P = 250 - 300d.
AW    Per |SB2, companion B6V, Delta(m) (companion - AW) = 2.8m vis.
AX    Per |Epoch of Min is given. The variability with Delta(m) up to
AX    Per |0.7m pg is caused probably by the orbital motion. Outburst
AX    Per |activity is superimposed.
AY    Per |d = 0.009P.
BE    Per |In the region of the open cluster CR 39.
BI    Per |In the region of the open cluster Berk 9.
BL    Per |P = 125 - 130d.
BM    Per |[Fe/H] = -0.04.
BP    Per |Min II = Min I. In the region of the open cluster
BP    Per |Cr 39.
BU    Per |Max brightness var, P = 8.1yr [01085]. In the region of
BU    Per |the open cluster h, khi Per.
CC    Per |Min II 14.1.
CI    Per |P var (3.35d - 3.40d), possibly with a period of 4000d.
CI    Per |The light curve shape var.
CK    Per |d = 0.05P:.
CM    Per |d = 0.052P. In the region of the open cluster Stock 2.
CO    Per |In the region of the open cluster Stock 2.
CR    Per |Elements need confirmation. In the region of the open
CR    Per |cluster Stock 2.
CS    Per |In the region of the open cluster Stock 2.
CZ    Per |In the region of the open cluster h, khi Per.
DE    Per |d = 0.01P?
DF    Per |In the region of the open cluster h, khi Per.
DG    Per |d = 0.021P.
DK    Per |The depth of Min II 0.05m. In the region of the open
DK    Per |cluster h, khi Per.
DM    Per |Min II 8.02, DII = 0.17P.
DM    Per |Depths of Minima, the shape of Min II var.
DM    Per |In the region of the open cluster h, khi Per.
DO    Per |In the region of the open cluster h, khi Per.
DP    Per |In the region of the open cluster h, khi Per.
DR    Per |In the region of the open cluster h, khi Per.
DS    Per |In the region of the open cluster h, khi Per.
DT    Per |In the region of the open cluster h, khi Per.
DU    Per |In the region of the open cluster h, khi Per.
DV    Per |Min II 14.5.
DY    Per |In the region of the open cluster Tr 2.
DZ    Per |Min II 14.7. In the region of the open cluster Tr 2.
EL    Per |Before JD2428900 Max = 2427980 + 167d*E;
EL    Per |during JD2428900 - 31000 - see Table.
EO    Per |IR excess?
ER    Per |Mean brightness var, P ~900d.
EU    Per |Min brightness var, P ~900d.
EW    Per |Superimposed waves 70d - 180d.
EW    Per |In the region of the open cluster Stock 4.
EX    Per |Min II 12.5.
FM    Per |VB A (B 12.1m, 3", 285deg). P var? Max = 2429982.268 +
FM    Per |0.489199d*E (JD2428000 - 30600);
FM    Per |During JD2433700 - 36000 - see Table.
FR    Per |In the region of the open cluster NGC 1528.
FV    Per |Cycles 300 - 350d, 1800d:.
FX    Per |d = 0.04P. In the region of the open cluster NGC 1582.
FY    Per |Possible periods 0.0702d, 0.4407d.
FY    Per |Photometric spectral type B1V.
FZ    Per |In the region of the open cluster h, khi Per.
GH    Per |P = 220d is possible.
GK    Per |SB2 (sdBE + K2IVp).
GK    Per |The following types of activity are being observed after
GK    Per |the return to the normal brightness: rapid irregular
GK    Per |variations (Delta(m) ~0.1m in several minutes); irregular
GK    Per |fluctuations from night to night (Delta(m) up to 0.3m);
GK    Per |slow irregular variations (Delta(m) = 1.5m in several
GK    Per |dozen days); bursts with light increase in 10d - 30d and
GK    Per |decrease in 10d - 40d, Delta(m) up to 3.5m, the mean
GK    Per |interval between bursts being delta(t) = 820d [09686,09788].
GK    Per |According to [10198], the radial velocities are
GK    Per |represented with the elements Max (Vr > 0) = 2444912.966 +
GK    Per |1.996803d*E (Kabs = 124 km/s, Kem = 34 km/s). According
GK    Per |to [10199], the 2d variation is modulated with a period
GK    Per |of 0.131623d, Max (delta(Vr)) ~2443787.995 (Kabs =
GK    Per |15 km/s, Kem = 20 km/s). During a burst the sinusoidal
GK    Per |modulation of X-ray flux was recorded,
GK    Per |Tmax = 24455555.67456 + 0.004066443d*E [09786].
GK    Per |ExpAnding envelope (0.454"/yr, 1948 - 1964;
GK    Per |0.432"/yr, 1964 - 1981, [09787]).
GP    Per |[A/H] = -0.5.
GQ    Per |According to [00021], Sp K0.
HQ    Per |[A/H] = -0.3.
HS    Per |In the region of the open cluster Stock 4.
HV    Per |d ~0.03P.
HW    Per |Min II 13.3. Min II - Min I = 0.45P:.
HY    Per |Three of the four min in [01079] are not satisfied with the
HY    Per |elements.
HZ    Per |[A/H] = -0.8. B_V: +1.93, +2.34.
II    Per |Min II 13.6. In the region of the open cluster NGC 1582.
IK    Per |Min II 11.6.
IM    Per |Min II 12.7. The elements need confirmation. In the region
IM    Per |of the open cluster Cr 39.
IO    Per |H2O maser.
IP    Per |IR excess.
IQ    Per |dI = 0.02P. Min II 7.88, DII = 0.12P, dII = 0.03P,
IQ    Per |Min II - Min I = 0.53P. P var? VB A (B = BD + 47deg 921,
IQ    Per |9.30m, A0V np:, 39.3", 175deg); SB1.
IT    Per |dI = 0.06P. Min II 10.0, DII = 0.24P:, dII = 0.16P:.
IT    Per |VB (Delta(m) = 1.7m, 12", 37deg).
IT    Per |The range of the combined brightness is given.
IW    Per |SB1. Min II 5.83.
IX    Per |The depth of Min II 0.02m.
IX    Per |VB A (B 10.6m, 5", 208deg).
IZ    Per |Min II 8.3.
KK    Per |In the region of the open cluster h, khi Per.
KP    Per |Beat phenomenon: P1 - see Table,
KP    Per |A1 = 0.0323m B; P2 = 0.1980855d, A2 = 0.0235M B; P3 =
KP    Per |0.2270986d, A3 = 0.0072M B.
KR    Per |Min II 11.1.
KS    Per |SB (Porb = 360.47d).
KS    Per |The main component is a helium star. Besides the
KS    Per |semiregular variability (see Table), variations were noted
KS    Per |with P = 50 - 100 Min and Delta(m) of several hundredths
KS    Per |of a magnitude. IR excess. Variable polarization (P - 1%).
KT    Per |Quasi-periodic oscillations during outbursts: P =
KT    Per |22.9s - 29.5s [05959], 82s, 90s, 147s [09791], Delta(m)
KT    Per |up to ~0.01m.
KV    Per |[Fe/H] = -0.96. P var. Max = 2428950.400 + 0.24942d*E
KV    Per |(JD2428950 - 29200); since JD2429500 - see Table.
KW    Per |Min II 10.8. P var. Min = 2426295.450 + 0.931255d*E
KW    Per |(JD2423400 - 39500) [04009]; since JD2440000 - see Table.
KY    Per |In the region of the open cluster h, khi Per.
KZ    Per |In the region of the open cluster h, khi Per.
LL    Per |In the region of the open cluster h, khi Per.
LM    Per |In the region of the open cluster h, khi Per.
LN    Per |In the region of the open cluster h, khi Per.
LO    Per |In the region of the open cluster h, khi Per.
LP    Per |In the region of the open cluster h, khi Per.
LQ    Per |In the region of the open cluster h, khi Per.
LR    Per |Very red. In the region of the open cluster h, khi Per.
LX    Per |mu alpha = +0.0065s, mu delta = -0.063". Min II 8.38m.
LX    Per |DII = 0.05P. Migrating distortion wave:
LX    Per |P = 475d [09792], Delta(m) up to 0.04m.
MS    Per |Min II 12.1.
MX    Per |IR excess.
NP    Per |Min II 13.0.
NR    Per |P var. Max = 2416780 + 323.0d*E (JD2415750 - 24550);
NR    Per |Max = 2435060 + 340.2d*E (JD243350 - 35400);
NR    Per |since JD2436700 - see Table.
NU    Per |A close pair, var is the southern star.
OV    Per |D ~2h.
PP    Per |In the region of the open cluster h, khi Per.
PR    Per |In the region of the open cluster h, khi Per.
QR    Per |Red.
QU    Per |d = 0.03P.
QW    Per |Min II 14.7:.
QX    Per |Min II 16.1.
V0345 Per |In the nebula NGC 1579.
V0346 Per |In the nebula NGC 1579.
V0347 Per |In the nebula NGC 1579.
V0351 Per |In the region of the open cluster h, khi Per.
V0352 Per |In the region of the open cluster h, khi Per.
V0354 Per |In the region of the open cluster h, khi Per.
V0355 Per |In the region of the open cluster h, khi Per.
V0356 Per |In the region of the open cluster h, khi Per.
V0357 Per |In the region of the open cluster h, khi Per. P = 0.21955d
V0357 Per |is possible.
V0358 Per |In the region of the open cluster h, khi Per.
V0359 Per |In the region of the open cluster h, khi Per.
V0360 Per |In the region of the open cluster h, khi Per.
V0360 Per |Other possible periods: 0.40036d, 0.40154d.
V0361 Per |In the region of the open cluster h, khi Per.
V0363 Per |Red.
V0364 Per |Min II 15.6, Max II 14.8.
V0365 Per |Min II 14.3:.
V0376 Per |P2 = 0.09165d, A2 = 0.016m; P1 - see Table,
V0376 Per |A1 = 0.037m. A var.
V0380 Per |SB (Porb = 26d?). The epoch of Min light is given.
V0382 Per |In the region of the open cluster h, khi Per.
V0392 Per |The southern component of a very close pair.
V0394 Per |H2O maser.
V0395 Per |VB A (B 3.5", 90deg).
V0396 Per |In the region of the open cluster alpha Per.
V0396 Per |Observations are also satisfied by P ~1.678d. According
V0396 Per |to [07586], P = 2.4928d or 1.6857d.
V0397 Per |ADS 2859 B (A = X Per; B 22.5", 12deg).
V0398 Per |IN type is also possible.
V0403 Per |In the region of the open cluster h, khi Per.
V0409 Per |Epoch of Min is given.
V0423 Per |ADS 2433 A (B 11.9m, 30.8", 99.2deg); SB.
V0423 Per |Porb is given.
V0424 Per |In the region of the open cluster h, khi Per. IR excess.
V0425 Per |VB A(B 12.8m, 3.6", C 14.3m, 6.8"). In the region of
V0425 Per |the open cluster h, khi Per.
V0428 Per |According to [08639], type IS?
V0432 Per |Min II 11.6.
V0434 Per |Min II 14.9.
V0436 Per |Min II 5.74; Min II - Min I = 0.413P; D II = 0.03P.
V0437 Per |In the region of the open cluster NGC 744.
V0438 Per |In the region of the open cluster h, khi Per. VB (8.7m,
V0438 Per |10.9m, 1".2, 26deg).
V0438 Per |Min II 8.34. The range of combined brightness
V0438 Per |variation is given. The bright component is
V0438 Per |considered to be variable. This suggestion
V0438 Per |needs verification.
V0439 Per |In the region of the open cluster h, khi Per.
V0440 Per |In the region of the open cluster h, khi Per. ADS 1820
V0440 Per |A (B 14.5m, 8".3, 122deg).
V0449 Per |Min II 13.3.
V0451 Per |Min II 15.8.
V0459 Per |In the alpha Per cluster.
V0461 Per |In the alpha Per cluster.
V0462 Per |Min II 14.0.
V0465 Per |P2 = 0.030d is superimposed.
V0466 Per |Superposition of P1 = 5300d +- 250d, P2 = 475d +- 35d
V0466 Per |(Delta(m) = 1.1m), P3 = 0.26d (Delta(m) = 0.5).
V0468 Per |P1 = 925s, P2 = 1022s. mu = 0".29, p = 170deg.
V0469 Per |Changes of line profiles with periods 0.150d, 0.188d,
V0469 Per |0.304d, 0.476d, 0.608d, 1.88d [09814].
V0469 Per |In 1978/1979 non-radial pulsations were observed:
V0469 Per |P1 = 1.74d. P2 = 2.04d [04173,04180].
V0470 Per |VB A (B 18.8m B, 1" - 2").
V0471 Per |The central star of the planetary nebula M1-2 = VV8.
V0471 Per |According to [09815,09816], const.
V0547 Per |High proper motion (LTT 10610) not confirmed by HIPPARCOS data.
V0580 Per |The variability may be due to the fainter (B) component.
V0582 Per |A single deep minimum at the bottom of the small-amplitude
V0582 Per |(5.63 - 5.64) wave.
V0592 Per |VB (0".2, 197 deg, 1989.7).
bet   Per |Multiple system (Eclipsing pair = Algol AB; Algol C 4.7m,
bet   Per |Am, a = 0".10, Porb = 1.862a); Algol AB = ADS 2362 A
bet   Per |(B 12.7m, 57".5, 156deg, 1920). P var. P = 2.8673442d
bet   Per |(1784 - 1835); P = 2.8673012d (1835 - 1854);
bet   Per |P = 2.8672775d
bet   Per |(1854 - 1901); P = 2.8672967d (1901 - 1913);
bet   Per |P = 2.8672506d
bet   Per |(1913 - 1915) [06156]; Min I = 2424477.806 + 2.86730236d*E
bet   Per |(JD2420500 - 25000); Min = 2425917.203 + 2.86732697d*E
bet   Per |(JD2425000 - 277000); Min I = 2433194.454 + 2.86731667d*E
bet   Per |(JD2427700 - 33600); Min I = 2433928.4944 + 2.86732442d*E
bet   Per |(JD2433600 - 37000); Min I = 2437598.6766 + 2.86733732d*E
bet   Per |(JD2437000 - 42200); since JD2442200 - see Table.
bet   Per |Porb (Algol C) = 1.862a may be traced in the deviations;
bet   Per |a period of 32a may also be real. Depth of Min I var.
bet   Per |Variable polarization, changes in hydrogen line profiles,
bet   Per |sometimes emissions in the spectrum. Radio source with
bet   Per |frequent burst of different amplitude, faint X-ray source.
del   Per |Variable emission lambda 1650 A [06905]. Vr var,
del   Per |A = 16 km/s.
ksi   Per |In the far IR range (lambda = 10 mkm) Delta(m) > 1m. In
ksi   Per |the far IR range (lambda = 10 mkm ) Delta(m) > 1m; the
ksi   Per |variability is related to mass loss.
omi   Per |VB A (B 8.4m, 0.96'', 29.7deg,1972). Possible
omi   Per |superposition of BCEP type oscilations.
rho   Per |A slower variation of the mean light is possible.
rho   Per |mu alpha = 0.0111s, mu delta = -0.102''.
phi   Per |SB2. (Porb = 126.696d). v*sin(i) = 450km/s. A var (P ~Porb).
b     Per |SB2. Depths of minima differ by 0.03m. Third body? ,
b     Per |P = 701d. Radio source. In  the region of the open cluster
b     Per |NGC 1545.
R     Phe |P var. Max = 2405121 + 271.0d*E(JD2405000 - 11500);
R     Phe |Max = 2414570 + 266.26d*E(JD2414500 - 25500);
R     Phe |since JD2425500 - see Table.
T     Phe |P var. Max = 2411252 + 281.00d*E(JD2410000 - 30000);
T     Phe |since JD2430000 - see Table.
W     Phe |P var. Max = 2414960 + 328.65d*E(JD2414500 - 19500);
W     Phe |Max = 2424530 + 332.87d*E(JD2424500 - 30200);
W     Phe |since JD2436000 - see Table.
RS    Phe |P var?
RT    Phe |P = 208d?
RV    Phe |P var?; (k-b)2 = 0.06; Delta(S) = 8:
SX    Phe |mu = 0.894", ro = 163.1deg. P var. Max = 2433923.9618 +
SX    Phe |0.054964519d*E1 - 0.00337d*sin(2pi*(0.28503379*E1 + 0.074))
SX    Phe |(JD2433900 - 36900); since JD2436900 - see Table.
SX    Phe |There is a periodic term in the elements given in the
SX    Phe |Table: -0.00325*sin(2pi*(0.28503575*E2 - 0.107)). According
SX    Phe |to [09614] for epoch 1950.0 P0 = 0.054964509,
SX    Phe |P1 = 0.042772831, Pb = 0.1928355; dP0/dt = -87*10**(-13),
SX    Phe |dP1/dt = -174*10**(-13), dPb/dt = 2.46*10**(-10).
SX    Phe |P1/P0 = 0.778; 0.8m <= A <= 0.3m;
SX    Phe |0.2p <= M-m <= 0.4p. [Fe/H] = -0.6.
WW    Phe |Min II 12.7.
YZ    Phe |Min II 13.0.
AD    Phe |Min II 10.80. P var. Min I = 2436847.375 + 0.3799277*E
AD    Phe |(JD2428650 - 36850); since JD2436850 - see Table.
AE    Phe |Min II 8.19; 0.033p <= dI <= 0.05p; dII = 0.00.  The
AE    Phe |shape of the light curve varies with periods 55.9d and
AE    Phe |95.3d [09615]. P var. Min I = 2440857.8140 + 0.36237459*E
AE    Phe |(JD2438250 - 40870) [07388]; Min I = 2441969.57074 +
AE    Phe |0.36237186d*E (JD2440870 - 42000) [09616]; Min I =
AE    Phe |2442654.8201 + 0.3623741d*E (JD2441950 - 42660) [09533];
AE    Phe |since JD2443700 - see Table.
AG    Phe |Min II 8.95. P var. Min I = 2440415.231 + 0.7553429d*E
AG    Phe |(JD243800 - 40850); since JD2443750 - see Table.
AI    Phe |Min II 8.89; dI = 0.0035; Min II - Min I = 0.46p.
AU    Phe |Min II 13.0. According to [09517] the P value given in
AU    Phe |the Table is wrong.
AX    Phe |mu = 0.234", p = 70deg. Multiperiodical: P i = 606.8s,
AX    Phe |682.7s, 744.7s, 840.2s (Ai ~0.01m).
CG    Phe |Type RRC: is also possible.
gam   Phe |SB1 (P orb = 193.85d).
zet   Phe |VB A (B 7.0m, A7:, 0.46", 51.4deg, 1965.9; C 8.0m,
zet   Phe |F7V, 6.4"). Total light range of A and B components is
zet   Phe |given in the Table. Min II 4.22, MinII - MinI = 0.507p;
zet   Phe |dII = 0.02p.
iot   Phe |VB A (B 12.7m, 7.7", 270deg).
ksi   Phe |VB A (B 12.1m, 13.2", 253deg). Epoch of MinI(v) is given
ksi   Phe |in the Table. A(v) = 0.13m.
rho   Phe |Frequency analysis results see also in [09619,09620,9621].
psi   Phe |SB.
R     Pic |P var. Max = 2413413  +  165.8d*E (JD2413000 - 23600);
R     Pic |since JD2423600 - see Table. Light curve (1923 - 1953)
R     Pic |[01054].
S     Pic |P var. Max = 2413595  +  424.7d*E (JD2405500 - 23000);
S     Pic |since JD2423000 - see Table. OH emission.
U     Pic |P var. Max = 2428103.565  +  0.44036450*E (JD2414000 -
U     Pic |29000) [00353]; since JD2438400 - see Table. (k - b)2 =
U     Pic |0.17; Delta(S) = 3.
X     Pic |Min II 10.8
RR    Pic |Since 1965 periodic light variations were detected
RR    Pic |with A(B) = 0.33m and elements Max = 2438815.380 +
RR    Pic |0.14502545d*E. These variations are superimposed by
RR    Pic |others with A(B) = 0.036m and period ~15.6 min or
RR    Pic |15.4 min [09612]. There are also rapid oscillations
RR    Pic |with periods in the range 20 - 40s [09613].
RT    Pic |Not seen only on one plate; defect?
RV    Pic |Min II 9.79.
SU    Pic |Min II 10.4.
VW    Pic |Variability may be due to component B.
VZ    Pic |Kapteyn's star.
del   Pic |Min II 4.83.
R     Psc |P var. Max = 2418070 + 344.14d*E (JD2397070 - 27700);
R     Psc |Max = 2432866 + 347.1d*E(JD2427300 - 33000) - see Table.
S     Psc |P var. Max = 2406665 + 405.6d*E (JD2398944 - 2407100);
S     Psc |Max = 2415930 + 402.6d*E (JD2407100 - 16500); Max =
S     Psc |2421295 + 413.7d*E (JD2416500 - 21500) - see Table.
U     Psc |P var. Max = 2417230 + 172.71d*E (JD2407720 - 18000);
U     Psc |Max = 2423840 + 174.3d*E (JD2418000 - 24000) [00001];
U     Psc |Max = 2424527 + 170.3d*E (JD2423000 - 26100) [00960];
U     Psc |Max = 2432514 + 174.05d*E (JD2425000 - 33000) [00001];
U     Psc |since JD2433000 - see Table.
V     Psc |mu alpha = 0.0112s, mu delta = -0.215".
W     Psc |P var. Max = 2412690 + 189.08d*E (JD2412692 - 27100)
W     Psc |[01193];
W     Psc |since JD2435000 - see Table.
X     Psc |P var. Max = 2433474 + 357.3*E (JD24295000 - 38000); since
X     Psc |JD2438000 - see Table.
Y     Psc |P var. Min = 2410002.844 + 3.76582d*E (JD2410000 - 19700)
Y     Psc |[09707]; Min = 2425495.522 + 3.765903d*E
Y     Psc |(JD2423200 - 6300) [01072]; Min = 2430613.384 +
Y     Psc |3.7658895d*E
Y     Psc |(JD2427300 - 30620); Min = 2432865.357 + 3.7658405d*E
Y     Psc |(JD2430620 - 32900); Min = 2435693.452 + 3.7657765d*E
Y     Psc |(JD2432860 - 36600) [00001]; Min = 2441225.473 +
Y     Psc |3.765859d*E
Y     Psc |(JD2439000 - 42500) [06956]; Min = 2443142.29056 +
Y     Psc |3.7658491d*E (JD2442500 - 44000) [08593]; since JD2444000 -
Y     Psc |see Table.
RS    Psc |In the region of the galaxy NGC 251.
RT    Psc |Mean brightness varies with P2 = 533d. According to [08643]
RT    Psc |30d <= P1 <= 70d.
RU    Psc |[Fe/H] = -1.65. P var. [00752,09714] Max = 2415407.609 +
RU    Psc |0.3903008d*E (JD2414400 - 15700); Max = 2416022.660 +
RU    Psc |0.3902139d*E (JD2415700 - 16600); Max = 2417244.537 +
RU    Psc |0.3902878d*E (JD2416600 - 19200); Max = 2419936.853 +
RU    Psc |0.3903520d*E (JD2419200 - 22000); Max = 2425894.778 +
RU    Psc |0.3903016d*E (JD2422000 - 26200); Max = 2426214.829 +
RU    Psc |0.3903546d*E (JD2426200 - 27300); Max = 2427397.519: +
RU    Psc |0.3902216d*E (JD2427300 - 28000); Max = 2428165.524 +
RU    Psc |0.3903535d*E (JD2428000 - 29300); Max = 2429488.868: +
RU    Psc |0.3904577d*E (JD2429300 - 600) [00752]. Max = 2430053.353 +
RU    Psc |0.390202d*E (JD2430000 - 650); Max = 2430935.366 +
RU    Psc |0.390354d*E (JD2430600 - 940); Max = 2431331.307 +
RU    Psc |0.390457d*E (JD2430940 - 31350); Max = 2432119.417 +
RU    Psc |0.390346d*E (JD2431350 - 32120); Max = 2433162.250 +
RU    Psc |0.390283d*E (JD2432100 - 33200); Max = 2433905.311 +
RU    Psc |0.390261d*E (JD2433200 - 33910); Max = 2433905.311 +
RU    Psc |0.390321d*E (JD2433900 - 35430); Max = 2435429.502 +
RU    Psc |0.390412d*E (JD2435420 - 35800); Max = 2435781.265 +
RU    Psc |0.39027d*E (JD2435780 - 36130); Max = 2436501.361 +
RU    Psc |0.39032d*E (JD2436130 - 36510); Max = 2436534.190 +
RU    Psc |0.39043d*E (JD2436500 - 36850); Max = 2436845.351 +
RU    Psc |0.39025d*E (JD2436840 - 37200); Max = 2437181.358 +
RU    Psc |0.39031d*E (JD2437180 - 37610); Max = 2437994.329 +
RU    Psc |0.39026d*E (JD2437610 - 38000); [00001].
RU    Psc |Max = 2438303.950 + 0.39040d*E (JD2438000 - 38400) [03879].
RU    Psc |Max = 2438375.409 + 0.39027d*E (JD2438370 - 38650) [00001].
RU    Psc |Max = 2439435.2421 + 0.390385d*E (JD2438650 - 39500)
RU    Psc |[09713]. Max = 2439435.242 + 0.390313d*E (JD2439430 - 39800);
RU    Psc |Max = 2439771.3049 + 0.39046d*E (JD2439770 - 40140) [00001].
RU    Psc |Since JD2440140 - see Table. According to [03569] A var
RU    Psc |with P = 28.8d.
RV    Psc |Min II 12.0.
RY    Psc |(k-b)2 = 0.03, Delta(S) = 7. P var. Max = 2419677.268 +
RY    Psc |0.52971027d*E (JD2414000 - 22000); Max = 2425148.192 +
RY    Psc |0.52972643d*E (JD2422000 - 25500) [01337]; Max =
RY    Psc |2425508.390 + 0.5297291d*E (JD2425500 - 40000);
RY    Psc |Max = 2441538.476 + 0.52972911d*E (JD2441000 - 41650)
RY    Psc |[07984]; since JD2442660 - see Table.
RZ    Psc |Algol-like.
SS    Psc |(k-b)2 = 0.19; Delta(S) = 2. Blazhko effect:
SS    Psc |-0.04d <= O-C <= +0.04d; Min(O-C) = 2437520 + 136d*E
SS    Psc |[09731].
SU    Psc |Min II 11.3.
SW    Psc |P var. Max = 2425177.298 + 0.5212844d*E (JD2419670 -
SW    Psc |25200) [04191]; Max = 2425177.256 + 0.5212642d*E
SW    Psc |(JD2425170 - 38000) [03506]. Since JD2438600 - see Table.
SW    Psc |There is a periodic term in the elements given in the
SW    Psc |Table: + 0.0132d*sin(5.440deg*(E + 2)). Blazhko effect
SW    Psc |(Pi = 34.5d).
SX    Psc |P var. Min = 2427811.357 + 0.825882d*E (JD2425580 - 36000)
SX    Psc |[01218]; Min = 2437202.453 + 0.825877d*E
SX    Psc |(JD2436000 - 39900)
SX    Psc |[00001]; since JD2439800 - see Table.
SZ    Psc |Min II 7.38. P var.
SZ    Psc |There is a square term in the elements given in the Table:
SZ    Psc |-0.113d*10**(-6)*E**2.
TY    Psc |Porb = 0.080d [09735].
TY    Psc |The cycle of supermaxima is 370d [09675].
UU    Psc |VB A (B 7.60m, F4V, 11.5", 148deg, 1966.9). Min II 6.04;
UU    Psc |Min II - Min I = 0.55P.
UU    Psc |Elliptical orbit and rotation of the line of apsides are
UU    Psc |possible.
UV    Psc |Min II 9.54. P var. Min I = 2424134.574 + 0.8610475d*E
UV    Psc |(JD2414600 - 24150) [00001]; Min I = 2428038.555 +
UV    Psc |0.861046d*E (JD2424150 - 36700) [02924];
UV    Psc |since JD2436700 - see Table. The shape of the light
UV    Psc |curve varies.
UW    Psc |Min II 11.0:.
UZ    Psc |SB1 (Porb > 1 yr [05751]).
VZ    Psc |Mu = 0.43", P =  65deg. Min II 10.43.
WW    Psc |VB A (B 13.1m, 31").
WX    Psc |OH, H2O, SiO maser.
ZZ    Psc |P1 = 612s, P2 = 816s [07476].
ZZ    Psc |Nonradial modes [08467].
AG    Psc |P (Vr) = 0.055d.
AH    Psc |The star was seen in 1854 - 60; since 1862 it was not
AH    Psc |observed.
AO    Psc |Epoch of Max brightness is given. Light variations with
AO    Psc |Porb = 0.1496263d are superimposed by variations with
AO    Psc |P = 858.6861s and twice smaller amplitude (Max =
AO    Psc |2444815.00276 + 0.009938496d*E; M-m = 0.54P), and
AO    Psc |also by still smaller oscillations with P = 805.2059s
AO    Psc |(Max = 2444815.00294 + 0.009319513d*E). The last period
AO    Psc |is the X-ray impulse period which is equal to
AO    Psc |the period of rotation of the compact object (probably
AO    Psc |a white dwarf).
R     PsA |P var. Max = 2417385 + 293.00d*E (JD2405000 - 26000);
R     PsA |Max = 2432896 + 291.50d*E (JD2426000 - 38000);
R     PsA |since JD2438000 - see Table.
S     PsA |P var. Max = 2417853 + 271.0d*E (JD2411000 - 18000);
S     PsA |Max = 2426880 + 273.6d (JD2418000 - 27000); Max =
S     PsA |2434714 + 270.3d (JD2427000 - 35000); since
S     PsA |JD2434000 - see Table.
X     PsA |Min II 14.2.
RW    PsA |Min II 11.63.
TX    PsA |VB B (A 13.0m pg; B 37", 131deg); mu = 0.22", p = 117deg.
pi    PsA |SB (Porb = 178.3177d [05769]).
R     Pup |In the region of the open cluster NGC 2439.
U     Pup |P var. Max = 2415090 + 314.26d*E (JD2408000 - 22800);
U     Pup |since JD2422800 - see Table.
V     Pup |VB A (B 10.0m, 7", 0, 70deg; C 11.0m, 19.0", 48deg).
V     Pup |Min II 4.82. P var. IO - CI < 0.02d.
W     Pup |P var. Max = 2420990 + 120.68d*E (JD2412500 - 23600);
W     Pup |Max = 2424725 + 119.9d*E (JD2423600 - 26300);
W     Pup |Max = 2432200 + 120.68d*E (JD2426300 - 40800);
W     Pup |since JD2440800 - see Table.
X     Pup |P var. Max = 2414889.8 + 25.939d*E (JD2408800 - 16000);
X     Pup |Max = 2435188.76 + 25.9610d*E (JD2419000 - 35190)
X     Pup |[02392]; Max = 2436279.50 + 25.97d*E
X     Pup |(2435190 - 38000) [00001]; since JD2438000 - see Table.
Z     Pup |OH, H2O, SiO emission.
Z     Pup |P var. Max = 2424256 + 513.90d*E (JD2413900 - 24500);
Z     Pup |since JD2424500 - see Table.
RS    Pup |Surrounded by the reflecting nebulosity with a radius of
RS    Pup |1.4' [09634]. P var. Max = 2419186.3 + 41.337d*E
RS    Pup |(JD2414000 - 24000) [02049]; Max = 2427083.613 + 41.414d*E
RS    Pup |(JD2425800 - 28300) [02440]; Max = 2434823.23 + 41.38535d*E
RS    Pup |(JD2433750 - 34900) [09636]; since JD2435700 - see Table.
RW    Pup |P var. Max = 2430175 + 332.5d*E (JD2424500 - 30200)
RW    Pup |[00001]; since JD2435800 - see Table.
RX    Pup |Light curve (1890 - 1925) [01265].
RX    Pup |Mira type component light variations are observed in the
RX    Pup |infrared region of spectrum: Max = 2444530 + 580d*E,
RX    Pup |3.99m - 6.00m J, M - m = 0.50P [09518].
ST    Pup |[A/H] = -0.9.
ST    Pup |The light curve shape and the period vary strongly:
ST    Pup |0.10P < M - m < 0.30P; 17.4d < P < 19.19d.
ST    Pup |P = 19.188d (JD2415000 - 17000); 18.949d
ST    Pup |(JD2417000 - 18000), 18.8065d (JD2418000 - 19000),
ST    Pup |18.721d (JD2419000 - 20000), 18.714d (JD2420000 - 21000),
ST    Pup |18.717d (JD2421000 - 22000), 18.6175d (JD2422000 - 23000),
ST    Pup |18.678d (JD2423000 - 24000), 18.735d (JD2424000 - 25000),
ST    Pup |18.796d (JD2425000 - 26000), 18.817d (JD2426000 - 27000)
ST    Pup |[01266]. Max = 2427779.6 + 18.846d*E (JD2427000 - 28000)
ST    Pup |[01266]; Max = 2428893.9 + 18.885d*E (JD2428000 - 29000)
ST    Pup |[00016]; Max = 2429697.51 + 19.188d*E (JD2429000 - 30000)
ST    Pup |[01266]. P = 19.142d (JD2430000 - 31000),
ST    Pup |19.145d (JD2431000 - 32000) [01266].
ST    Pup |Max = 2435395.430 + 18.559d*E (JD2435160 - 500)
ST    Pup |[06006]; Max = 2435617.45 + 18.8864d*E (JD2435500 - 5620)
ST    Pup |[02309]; Max = 243957.3 + 17.4d*E (JD2438700 - 39600)
ST    Pup |[06611]; since JD2444000 - see Table.
SV    Pup |P var. Max = 2419010 + 166.6d*E (JD2413660 - 18000);
SV    Pup |Max = 2423090 + 169.8d*E (JD2418000 - 23100);
SV    Pup |Max = 2426782 + 167.8d*E (JD2423100 - 27500);
SV    Pup |since JD2427500 - see Table.
SW    Pup |Min II 9.1; d = 0.029P.
TT    Pup |Min II 13.6.
TY    Pup |Min II 8.87.
UZ    Pup |Min II 10.0.
VV    Pup |mu = 0.100", P = 165.0deg.
VV    Pup |The epoch of light maximum is given. The mean
VV    Pup |brightness varies by 2 - 3m. Intervals of active light
VV    Pup |variation with amplitude up to 2m during maximal mean
VV    Pup |brightness are observed. During low activity intervals
VV    Pup |when amplitude is about 0.3m mean brightness is minimal;
VV    Pup |during this time the ellipsoidal light variations of the
VV    Pup |system are observed in the range 15.1m - 15.3m J with the
VV    Pup |elements Min = 2427889.6509 + 0.0697468256d*E [09644].
VV    Pup |The white dwarf rotation period is equal to the orbital
VV    Pup |period. There are flickerings. Spectrum description
VV    Pup |[09472,09645].
VW    Pup |P var. Max = 2425184.67 + 4.28405d*E (JD2422660 - 25600)
VW    Pup |[00973]; Max = 2435554.86 + 4.28519d*E (JD2425600 - 35600)
VW    Pup |[02309]; since JD2435500 - see Table.
VX    Pup |P1 = 2.1389d (A1 = 0.29m); A0 = 0.31m; P1/P0 = 0.71042.
VY    Pup |The depth of Min II 0.04m.
VZ    Pup |[A/H] = -0.3. P var. Max = 2434864.90 + 23.1640d*E
VZ    Pup |(JD2426700 - 35300) [02309]; since JD2435300 - see Table.
WW    Pup |P var. Max = 2424497.73 + 5.5159d*E (JD2423520 -
WW    Pup |26000) [00973]; since JD2426000 - see Table.
WX    Pup |P var. Max = 2435042.184 + 8.93825d*E (JD2422000 -
WX    Pup |35100) [02431]; since JD2435000 - see Table.
WZ    Pup |P var. Max = 2427861.33 + 5.02657d*E (JD2421100 -
WZ    Pup |29400) [02392]; since JD2429400 - see Table.
XX    Pup |P var. Max = 2426338.503 + 0.51719805d*E
XX    Pup |(JD2426300 - 39500) [03572]; since JD2441700 - see Table.
XX    Pup |(k - b)2 = 0.07. The spectral type according to CA II is
XX    Pup |given.
XY    Pup |Min II 9.4; d = 0.042P.
XZ    Pup |Min II 7.90. P var. Min I = 2440629.7969 + 2.192383d*E
XZ    Pup |(JD2425850 - 41700) [00099]; since JD2441700 - see Table.
YY    Pup |The depth of Min II 0.05m.
AE    Pup |In the region of the open cluster Cr 173.
AF    Pup |Min II 13.5.
AG    Pup |Min II 10.9.
AH    Pup |The depth of Min II 0.05m.
AN    Pup |Min II 10.7.
AQ    Pup |VB A (B 11.13m, < 15"; C 12.83m, < 15"). [A/H] = -0.1.
AQ    Pup |The range of the variation of combined light is given.
AQ    Pup |P var. Max = 2429734.59 + 29.931d*E (JD2427500 - 33000)
AQ    Pup |[03474]; Max = 2433296.2 + 30.018d*E (JD2433000 - 35850)
AQ    Pup |[02474]; Max = 2436625.9 + 29.8568d*E
AQ    Pup |(JD2435850 - 36700) [03601]; Max = 2441760.63 + 30.032d*E
AQ    Pup |(JD2436600 - 42700) [09671]; since JD2443400 - see Table.
AR    Pup |The mean brightness varies with P = 1200d.
AS    Pup |In the region of the open cluster NGC 2546. P var.
AS    Pup |Max = 2416110 + 331.4d*E (JD2415460 - 26000); since
AS    Pup |JD2426000 - see Table.
AT    Pup |In the region of the open cluster NGC 2546.
AT    Pup |P var. Max = 2426758.205 + 6.6648d*E (JD2426700 - 35600)
AT    Pup |[02202]; since JD2435600 - see Table.
AU    Pup |Min II 9.28. P var. Min I = 2428111.304 + 1.126418d*E
AU    Pup |(JD2414700 - 28200) [00007]; since JD2439000 - see Table.
AV    Pup |Min II 11.0.
AW    Pup |VB A (B 11.7m, 3.7", 258deg). Period probably must be
AW    Pup |doubled.
AY    Pup |Min II 12.5.
AZ    Pup |Min II 10.1.
BB    Pup |(k - b)2 = 0.24; Delta(S) = 3.
BH    Pup |In the region of the open cluster Cr 173.
BI    Pup |In the region of the open cluster Cr 173.
BK    Pup |In the region of the open cluster Cr 173.
BL    Pup |Min II 14.2.
BN    Pup |In the region of the open cluster NGC 2533.
BP    Pup |Min II 12.3.
BQ    Pup |The shape of the light curve possibly varies.
BR    Pup |Min II 12.9.
BT    Pup |Min II 14.5. In the region of the open cluster NGC 2482.
BU    Pup |Min II 13.9. In the region of the open cluster NGC 2447.
BW    Pup |The depth of Min II 0.15m.
BX    Pup |In the region of the open cluster NGC 2482.
CE    Pup |P var? [07934].
CH    Pup |P var. Max = 2428465 + 491.0d*E (JD2428400 - 37300);
CH    Pup |since JD2437300 - see Table.
CO    Pup |P var? The epoch of light minimum is given.
CP    Pup |In 1981 the radius of the shell expanding with
CP    Pup |Vexp = 710 km/s was equal to 7" [09689,09559].
CX    Pup |d = 0.05P.
CY    Pup |d = 0.01P:; Min II 13.0.
CZ    Pup |Min II 13.1.
DD    Pup |Min II 14.6; Min II - Min I = 0.572P.
DE    Pup |Min II 12.9.
DF    Pup |Min II 12.8.
DK    Pup |Min II 13.0.
DM    Pup |Min II 13.7; Min II - Min I = 0.62P.
DN    Pup |Min II 13.5.
DO    Pup |Min II 13.3.
DR    Pup |Min II 13.3:.
DS    Pup |Min II 13.4.
DT    Pup |Min II 14.3.
EK    Pup |VB A (B 15", 270deg). P var? Max = 2427747.89 + 2.62587d*E
EK    Pup |(JD2425500 - 29500) [01343]; since JD2434500 - see Table.
EL    Pup |P > 1.3d? In the region of the open cluster NGC 2437.
EN    Pup |Min II 11.4.
EQ    Pup |Min II 10.9.
ES    Pup |According to [00412], Max = 2430377 + 187d*E.
ES    Pup |The elements given in the Table are valid in the interval
ES    Pup |JD2425600 - 29700.
EU    Pup |Min II 14.8.
FK    Pup |A var (P2 = 3000d). Strong SiC2 bands in the spectrum.
FM    Pup |Min II 14.2.
GG    Pup |S5/5.
GH    Pup |VB A (B 10", 195deg; C 16", 280deg; D 14", 315deg). P var.
GH    Pup |Max = 2425450 + 800d*E (JD2425300 - 28000); since
GH    Pup |JD2428700 - see Table. Very red.
GI    Pup |In the region of the open cluster NGC 2437.
GK    Pup |IN the region of the open cluster NGC 2437.
GN    Pup |VB A (B 16.5m, 10", 80deg).
GP    Pup |Min II 13.5.
GU    Pup |Min II 12.2.
GX    Pup |Min II 13.9. In the region of the open cluster Cr 173.
GY    Pup |Min II 12.3.
GZ    Pup |Min II 12.1.
HH    Pup |(k - b)2 = 0.14, Delta(S) = 1.
HI    Pup |Min II 11.0. In the region of the open cluster Cr 173.
HK    Pup |P var. Max = 2425925.732 + 0.7342532d*E
HK    Pup |(JD2425300 - 36600) [04127]; since JD2436600 - see Table.
HM    Pup |There is a shallow Min II.
HP    Pup |P var?
HW    Pup |P var? Max = 2429756.28 + 13.4532d*E (JD2427100 - 33000)
HW    Pup |[03551]; since JD2433000 - see Table.
KQ    Pup |In the open cluster NGC2422. SB2 (Porb = 9752d [03985]).
KT    Pup |Min II 13.4.
KW    Pup |Min II 11.8.
KX    Pup |Min II 13.04; 0.435P (1930) < Min II - Min I < 0.56P (1973)
KX    Pup |[03474,08094]; e = 0.15. Apsidal motion.
KY    Pup |Min II 11.1.
LN    Pup |Min II 12.9; Min II - Min I = 0.533P.
LO    Pup |Min II 13.9.
LP    Pup |d = 0.03P:.
LT    Pup |Min II 12.6.
MN    Pup |Min II 13.2.
MQ    Pup |Min II 9.39.
MT    Pup |RCB?
MW    Pup |Min II 9.2.
NO    Pup |VB A (BC 7.19m V, 8.1". 124deg (delta(M) = 0.0m, 0.20",
NO    Pup |275deg,
NO    Pup |1976)). Min II 6.66; Min II - Min I = 0.582P; e = 0.123.
NQ    Pup |S 4.5/2-.
NW    Pup |Porb = 1d.
NX    Pup |Connected with a cometary nebula.
OR    Pup |In the region of the open cluster NGC 2467.
OS    Pup |VB A (B 6.10m, 67.4").
OS    Pup |In the region of the open cluster C 0812-362.
OU    Pup |In the region of the open cluster IC 2391.
OX    Pup |In the region of the open cluster NGC 2451.
PS    Pup |The depth of Min II 0.028m.
PT    Pup |P2 = 0.168377d. A (lambda 1550) = 0.043m;
PT    Pup |0.015m < A(B) < 0.035m.
PU    Pup |VB (5.2m, 5.6m; 0.11", 43.6deg, 1927). Min II 4.74.
PV    Pup |VB B (A 6.1m; B 16.9", 340deg; C 10.5m, 100.4", 228deg).
PV    Pup |Min II 7.31; DII 0.10P; Min II - Min I = 0.47P.
PV    Pup |The light curve shape in Max and Min II varies.
PV    Pup |The deviations DB from the mean curve vary from -0.06m
PV    Pup |to +0.03m with the elements: Max (IDelta(B)I) =
PV    Pup |2440000.027458 + 1.92207d*E or Max (IDelta(B)I) =
PV    Pup |2440000.219470 + 0.48003d*E.
PW    Pup |Min II 9.54; d = 0.095P. In the region of the open
PW    Pup |cluster NGC 2439.
QS    Pup |0.008m <= A(u) <= 0.015m.
QT    Pup |Probably a member of the open cluster NGC 2477.
QU    Pup |P2 = 0.1680d or 0.2019d; 0.010m <= A(u) <= 0.040m.
QV    Pup |May be a member of the open cluster NGC 2489.
V0360 Pup |Type ACV: is also possible.
V0364 Pup |The preceding component of the northern star in the system of two
V0364 Pup |CoD-CPD objects, COD-36 3425 and CoD-36 3426 (CPD-36 1171 and CPD-36
V0364 Pup |1172).  The cross-identifications of these CoD and CPD objects differ
V0364 Pup |from one source to another; our adopted identification is based on the
V0364 Pup |paper editions of the catalogs.
V0376 Pup |Type ACV: is also possible.
V0378 Pup |Type BE is also possible.
V0393 Pup |SB, Porb = 2.5248d.
V0419 Pup |Not a nearby star (despite having a Gl number).
omi   Pup |Type EA: is also possible.
rho   Pup |VB A (B 13.7m, 29.6", 15deg). [Fe/H] = +0.13. P var.
rho   Pup |Max = 2435552.807 + 0.14088141d*E (JD2413900 -
rho   Pup |37500) [09756]; Max = 2439887.843 + 0.14088141d*E
rho   Pup |(JD2439800 - 43700); since JD2444000 - see Table.
L   2 Pup |VB A (B 11.5m, 62", 214deg); mu = 0.34", P=18deg. H2O,
L   2 Pup |SiO maser.
S     Pyx |P var. Max = 2411770 + 206.60d*E (JD2405500 - 23700);
S     Pyx |Max = 2423765 + 207.0d*E (JD2423700 - 29600);
S     Pyx |since JD2429600 - see Table.
T     Pyx |Previous outbursts were observed in 1890, 1902, 1920, 1944.
RR    Pyx |A close companion 14.5m.
RZ    Pyx |Min II 9.69.
SU    Pyx |d = 0.016P.
TT    Pyx |P = 3.031556d?
TV    Pyx |Depth of Min II 0.05m.
TX    Pyx |Min II 9.8.
TY    Pyx |Min II 7.48.
TZ    Pyx |Min II 11.1.
UZ    Pyx |VB A (B 7.61m, 110", 180deg).
VV    Pyx |VB A (B 8.58m, 0.3").
VV    Pyx |Range of the variation of combined light is given.
VV    Pyx |Min II 7.03; DII = 0.08P; Min II - Min I =
VV    Pyx |0.48P. Min II = 2444622.86709 + 4.5961766d*E.
VV    Pyx |Apsidal motion (P = 3200 yr).
VW    Pyx |The nucleus of the planetary nebula K1-2.
VW    Pyx |The range of the variations of combined light:
VW    Pyx |15.7 - 17.4 pg. The value of P close to
VW    Pyx |that found by bond [09767] and the epoch of Max brightness
VW    Pyx |are given in the Table.
R     Ret |P var. Max = 2403013 + 280.0d*E (JD2403000 - 13900);
R     Ret |Max = 2423317 + 276.68d*E (JD2413900 - 25300);
R     Ret |Max = 2430008 + 279.7d*E (JD2425200 - 30020);
R     Ret |since JD2430000 - see Table.
T     Ret |Mean brightness varies with P = 200d.
X     Ret |(k - b)2 = 0.09. P var. Max = 2427425.47 + 0.4920d*E
X     Ret |[00357]; Max = 2434334.611 + 0.492011d*E (JD2434300 - 600)
X     Ret |[00080]; since JD2434600 - see Table.
X     Ret |The shape of the light curve varies. Blazhko effect:
X     Ret |Pi >= 45d; 0.13P <= M - m <= 0.23P [00080].
R     Sge |P var (70.07d <= P <= 71.24d [09769]. Period variation
R     Sge |study [00767]. The elements given in the Table are valid
R     Sge |since JD2434000. The mean brightness varies:
R     Sge |Min = 2414402 + 1112.d*E [01357].
S     Sge |SB1 (Porb = 675d [01358]). P var. Max = 2409863.32 +
S     Sge |8.381968d*E (JD2406600 - 18000); since
S     Sge |JD2418000 - see Table.
U     Sge |VB A (B 9.6m, 92.0", 318deg). Min II 6.71;
U     Sge |0.014P <= dI <= 0.024P. In the region of the open cluster
U     Sge |Col 399. Not a member of the cluster. P var [06224,08608].
U     Sge |Mean elements are given in the Table representing
U     Sge |epochs of Min within  +-0.008P. The shape of the light
U     Sge |curve varies.
V     Sge |VB A (B 13.9m, 9.7", 267deg); SB2 (K1 = 320 km/s,
V     Sge |K2 = 85 km/s). P var? The depth of eclipses
V     Sge |varies from 0.6m to 1.3m. The mean brightness outside
V     Sge |eclipses varies. There are also flares with amplitudes up
V     Sge |to 3m and small light variations with a time
V     Sge |scale of minutes, dozens of minutes and a few days.
V     Sge |spectrum description [03593,09472].
X     Sge |VB A (B 13.18m, 6", 248deg).
Z     Sge |V1 (NGC 6838, M71). Globular cluster member. P var.
Z     Sge |Max = 2437870 + 175.3d*E (JD2437000 - 38700); since
Z     Sge |JD2438700 - see Table.
RS    Sge |The mean brightnese varies: Max = 2435999 + 1124d*E [08104].
RS    Sge |Two Algol-like light weakenings were also
RS    Sge |observed: JD2444837.22, 2444865.17 [09727].
RW    Sge |P var. according to [01363] Max = 2424289 + 429d*E. Since
RW    Sge |JD2434000 - see Table.
RZ    Sge |Porb ~97m [09771]. Mean cycle is given according to [09785].
RZ    Sge |Supermaxima are repeated with the cycle 266d. The period
RZ    Sge |of superhumps decreases from 101.3m till 100.8m.
SY    Sge |Min II 10.7. P var. Elements given in the Table are valid
SY    Sge |in the interval JD2425800 - 38300.
TU    Sge |d = 0.035P.
TX    Sge |P var. Max = 2425002 + 155.0d*E (JD2414900 - 25100);
TX    Sge |since JD2425000 - see Table.
UU    Sge |VB A (B 16.5m B, 4", 90deg). The nucleus of the planetary
UU    Sge |nebula Abell 63. Min II 14.41; d = 0.019P.
UU    Sge |The range of the combined light variation is given.
UU    Sge |The actual depth of Min I is about 4.3m. Large reflection
UU    Sge |effect.
UZ    Sge |Min II 11.6:. P var. Min I = 2429961.231 + 2.215750d*E
UZ    Sge |(JD2429000 - 41600); since JD2441600 - see Table.
VZ    Sge |VB A (B 12m, 28.2", 206deg).
WY    Sge |Nova Sge 1783 (Max JD2372494:). Min I = 2445137.8993 +
WY    Sge |0.1536342d*E; D = 0.16P. Brightness outside eclipses is
WY    Sge |usually ~18.7m, the depth of the eclipses is ~ 1.5 - 2m.
WY    Sge |At present outbursts by 1.6m are sometimes observed
WY    Sge |similar to the UG type variable outbursts, as well as
WY    Sge |rapid flickering of light [09708].
WZ    Sge |Nova Sge 1913, 1946, 1978. VB A (B 15.76m B, 7", 280deg).
WZ    Sge |Really it is not a nova. Three outbursts were registered
WZ    Sge |up to day: JD2420094, 32001, 43844 [09710,09711].
WZ    Sge |There are superhumps on the light curve during the
WZ    Sge |outburst with 0.057250d >= P >= 0.05714d (A=0.3m V)
WZ    Sge |[09710,09776]. There are light variations between
WZ    Sge |the outbursts (A = 0.14m - 0.3m). During some of light
WZ    Sge |weakenings Algol-like eclipses are observed (A = 0.2m)
WZ    Sge |with the elements: Min I = 2437547.72845 + 0.0566878455d*E
WZ    Sge |[09774]; D = 0.04P. d = 0.02P. There are also rapid light
WZ    Sge |oscillations (A <= 0.01m). The periods of these
WZ    Sge |oscillations before the 1978 outburst were 28.98s and
WZ    Sge |27.87s [09774], but after this outburst - 28.95963s [09775].
WZ    Sge |According to [09777], in 1976 - 78 these oscillations were
WZ    Sge |represented by the elements: Max = 2443311.790250 +
WZ    Sge |0.00032254826d*E + 9.8d*10**(-16)*E**2.
XY    Sge |According to [03705] the spectrum is earlier than M0.
AG    Sge |P = 117d?
BR    Sge |d = 0.030P.
CP    Sge |Min II 13.3.
CU    Sge |Min II 11.3.
CW    Sge |Min II 11.7. P var? The shape of the light curve varies.
CZ    Sge |Min II 15.2.
DH    Sge |The shape of the light curve varies (1.1m <= A <= 1.7m).
DH    Sge |P var. Max = 2427612.509 + 0.4695844D*E (JD2427600 -
DH    Sge |38800) [04027]; since JD2438800 - see Table.
DH    Sge |Blazhko effect disappeared after the period change
DH    Sge |(A = 1.1m).
DI    Sge |P var. Max = 2427929 + 203.0d*E (JD2427500 - 30200)
DI    Sge |[02641]; since JD2437100 - see Table.
DK    Sge |Min II 13.0.
DL    Sge |Min II 11.5.
DM    Sge |Min II 11.6.
DP    Sge |P var. Max = 2427985.464 + 0.4883395d*E (JD2427985 - 33000);
DP    Sge |Max = 2432855.191 + 0.4883339d*E (JD2433000 - 40775);
DP    Sge |since JD2440775 - see Table.
DQ    Sge |Min II 14.8.
DS    Sge |Min II 16.0:.
DT    Sge |d = 0.05P:.
EH    Sge |VB A (B 15.6m).
EI    Sge |Min II 14.6.
ER    Sge |P var. Max = 2430515.460 + 0.4184209d*E
ER    Sge |(JD2427000 - 38400);
ER    Sge |Max = 2438443.388 + 0.4184356d*E (JD2438400 - 41800);
ER    Sge |since JD2441800 - see Table.
FF    Sge |d = 0.03P; Min II 13.0.
FG    Sge |VB A (B 14.2m, 8", 100deg). The central star of the
FG    Sge |planetry nebula PK 60deg (diameter 36", the age about 6000
FG    Sge |years). The brightness of the star steadily increased from
FG    Sge |13.6 pg in 1894 to the maximum in 1967, and then is
FG    Sge |steadily decreasing. In 1982 it was 11.0 B. In 1967 the
FG    Sge |strong absorption lines of rare earth elements appeared
FG    Sge |in the spectrum. The spectral class steadily becomes
FG    Sge |later. The signes of new planetary nebula ejection were
FG    Sge |observed. In 1962 the star entered the instability
FG    Sge |strip in the Mv, B-V diagram and began to pulsate
FG    Sge |with a small amplitude and increasing period: Min(V) =
FG    Sge |2442629 + 59.83d*E + 1.126d*E**2 (JD2442600 - 44530).
FG    Sge |In twenty years the period increased from 50d to 134d,
FG    Sge |the amplitude of pulsations changed from 0.2mV to 0.5mV;
FG    Sge |now it decreased again to 0.2mV, and the period is only
FG    Sge |90d [09780].
FH    Sge |Min II 13.5.
FL    Sge |There is a close companion 14m. In the minimum probably
FL    Sge |fainter than 15.9m.
FO    Sge |P var. Max = 2427578.0 + 67.8d*E (JD2427570 - 28120);
FO    Sge |Max = 2428134.4 + 72.7d*E (JD2428120 - 30150);
FO    Sge |since JD2430150 - see Table.
FP    Sge |Min II 14.9. P = 0.32100275d?
FT    Sge |P.K.55-1 deg 2. Not a planetary nebula.
FU    Sge |Min II 15.8.
FX    Sge |In the region of the globular cluster M71 (NGC 6838).
GI    Sge |Red.
GN    Sge |Min II 10.6.
GP    Sge |Red.
GY    Sge |P var. Max = 2431264.49 + 51.497d*E (JD2429490 - 34900)
GY    Sge |[07199]; Max = 2433787.42 + 51.5991d*E (JD2433600 - 37280),
GY    Sge |Max = 437911.04 + 51.2524d*E (JD2437280 - 40510) [06172];
GY    Sge |since JD2444450 - see Table.
HH    Sge |The cycles 23 - 26d and 300d are observed.
HM    Sge |VB A (B 14.20m, 10", 182deg). The brightness increased
HM    Sge |from 17.2m up to 11.3m pg in the interval JD2442280 -
HM    Sge |42650. Then the light variations in the infrared region
HM    Sge |appeared with P = 550d [09721,09783] and A(K) = 1.5m.
HM    Sge |Radio and X-ray source.
IR    Sge |SF star in a close pair.
LN    Sge |SF star in a close pair.
MV    Sge |Possible member of the globular cluster Palomar 10.
MZ    Sge |Possible member of the globular cluster Palomar 10.
PT    Sge |P component of a close pair.
V0339 Sge |Extremely metal-weak.
del   Sge |VB A (B, A = 0.04", P = 7 yr); SB2 (Porb = 3725d [09789]).
del   Sge |The last superior conjunction of the B-star and its
del   Sge |atmospheric eclipse was in March - April 1980 [09726].
R     Sgr |P var. Max = 2405776 + 271.0d*E (JD2399500 - 2407500);
R     Sgr |Max = 2407115 + 264.2d*E (JD2407100 - 9500);
R     Sgr |Max = 2418125 + 269.65d*E (JD2409500 - 19500);
R     Sgr |Max = 2433137 + 267.90d*E (JD2419500 - 36000);
R     Sgr |since JD2436000 - see Table.
S     Sgr |P var. Max = 2401029 + 230.6d*E (JD2401000 - 10000);
S     Sgr |Max = 2411638 + 229.2d*E (JD2410000 - 19500);
S     Sgr |Max = 2422222 + 232.81d*E (JD2419500 - 27000);
S     Sgr |since JD2427000 - see Table.
T     Sgr |Companion F3IV (ro < 0.8"). P var.
T     Sgr |Max = 2409013 + 385.1d*E (JD2401500 - 10500);
T     Sgr |Max = 2414582 + 399.0d*E (JD2413000 - 17500);
T     Sgr |Max = 2424363 + 387.9d*E (JD2417500 - 25500);
T     Sgr |since JD2425500 - see Table.
T     Sgr |S 5/6-e. There are Te lines and a very strong
T     Sgr |Li lambda 6708 line in the spectrum.
U     Sgr |The member of the open  cluster M25 (IC 4725).
U     Sgr |P var. Max = 2416628.046 + 6.744925d*E (JD2404480 - 30115)
U     Sgr |[00765]; since JD2430115 - see Table. [A/H] = 0.1.
W     Sgr |VB A (A 9.2m, 0.116", 153.3deg, 1976.477; B 13.5m, 33.4",
W     Sgr |233deg; C 13.5m, 47.9", 101deg). P var.
W     Sgr |Max = 2403198.39 + 7.594695d*E (JD2403100 - 34500); since
W     Sgr |JD2434500 - see Table.
X     Sgr |P var. Max = 2410006.22 + 7.01206d*E (JD2403000 - 17000);
X     Sgr |Max = 2424248.11 + 7.01245d*E (JD2417000 - 34500); since
X     Sgr |JD2434500 - see Table.
Y     Sgr |In the region of the open cluster M25 (IC 4725).
RR    Sgr |P var. Max = 2410008 + 336.0d*E (JD2410000 - 17100)
RR    Sgr |[09794]; Max = 2422755 + 332.73d*E (JD2422700 - 32100)
RR    Sgr |[00960]; since JD2432100 - see Table. OH, H2O emission.
RS    Sgr |VB A (B 9.65m V, 39.0", 86deg). Min II 6.28.
RT    Sgr |P var. Max = 2412759 + 303.1d*E (JD2412700 - 8300)
RT    Sgr |[00960]; Max = 2425588 + 308.8d*E (JD2422800 - 26700);
RT    Sgr |Max = 2428034 + 303.8d*E (JD2426700 - 33500);
RT    Sgr |since JD2433500 - see Table.
RU    Sgr |P var. Max = 2413062 + 242.3d*E (JD2410150 - 16700)
RU    Sgr |[00960]; Max = 2423670 + 242.3d*E (JD2422500 - 24500);
RU    Sgr |Max = 2428200 + 237.6d*E (JD2424500 - 28800); since
RU    Sgr |JD2428800 - see Table.
RV    Sgr |P var. Max = 2411206 + 319.3d*E (JD2410200 - 17000)
RV    Sgr |[00960]; Max = 2429032 + 321.3d*E (JD2422600 -
RV    Sgr |29500); since JD2429500 - see Table.
RW    Sgr |P var. Max = 2413798 + 189.0d*E (JD2413700 - 23000);
RW    Sgr |Max = 2431998 + 190.87d*E (JD2423000 - 33500);
RW    Sgr |since JD2433500 - see Table.
RX    Sgr |P var. Max = 2417730 + 330.3d*E (JD2413000 - 18500);
RX    Sgr |Max = 2420122 + 346d*E (JD2418500 - 20150);
RX    Sgr |Max = 2420122 + 323d*E (JD2420100 - 22200);
RX    Sgr |Max = 2424120 + 345d*E (JD2422200 - 24200);
RX    Sgr |Max = 2428785 + 332.2d*E (JD2424000 - 31500);
RX    Sgr |since JD2431500 - see Table.
RY    Sgr |VB A (B 15.69m, 12"). There are pulsational light
RY    Sgr |variations (0.1m < A < 1.5m) with the elements:
RY    Sgr |Max = 2433670 + 38.6056d*E - 78d*10**(-5)*E**2.
RY    Sgr |light curve [09798,09799]; spectrum description [06261].
ST    Sgr |S 6/3-e.
SU    Sgr |VB A (B 13.5m, 1.0", 240deg, 1932.45).
SU    Sgr |earlier P = 88d was observed [00017].
SV    Sgr |In the nebula M8 (NGC 6523).
SW    Sgr |P var. Max = 2416338 + 290.3d*E (JD2414000 - 16500);
SW    Sgr |Max = 2428507 + 288.5d*E (JD2422500 - 29000);
SW    Sgr |Max = 2429088 + 293.5d*E (JD2429000 - 33000);
SW    Sgr |since JD2433000 - see Table.
SX    Sgr |Min II 9.62; d = 0.05P. P var. Min I = 2429114.249 +
SX    Sgr |4.15395762d*E (JD2410000 - 29150) [00007];
SX    Sgr |since JD2429000 - see Table.
SY    Sgr |In the region of the nebula S188.
SZ    Sgr |VB A (B 12.5m V, 2.0", 212deg.)
VV    Sgr |In the region of the open cluster NGC 6494. OH, H2O
VV    Sgr |emission.
VX    Sgr |P var; 1m <= A <= 6m. SIO, H2O, OH maser.
VX    Sgr |Light curve (1935-1969) [06615].
VY    Sgr |[A/H] = 0.5.
WX    Sgr |VB A (B 12.5m, 0.4", 88deg). P var. Min = 2419317.259 +
WX    Sgr |2.129095d*E (JD2419300 - 24700) [00457]; Min =
WX    Sgr |2424729.418 + 2.129113d*E (JD2424700 - 39700)
WX    Sgr |[00279]; since JD2440000 - see Table.
WY    Sgr |Min II 10.3.
WZ    Sgr |The member of the open cluster C 1814-190. [A/H] = 0.4.
XX    Sgr |P var. Max = 2419189.730 + 6.424264d*E (JD2419100 - 30100)
XX    Sgr |[00637]; since JD2435000 - see Table.
XZ    Sgr |Min II 8.95; d = 0.022P. P var. Min I = 2420311.519 +
XZ    Sgr |3.275537d*E (JD2420300 - 28000) [01604]; Min I =
XZ    Sgr |2436440.137 + 3.27549d*E (JD2428000 - 37500)
XZ    Sgr |[02516]; Min I = 2441150.348 + 3.2755357d*E
XZ    Sgr |(JD2437500 - 41500) [07084]; since JD2441500 - see Table.
YY    Sgr |Min II 10.64; Min II = 2433075.8296 + 2.628463d*E
YY    Sgr |[02302]. Apsidal motion period is about 300 years.
AL    Sgr |P var. Max = 2425792 + 79.07d*E (JD2421000 - 26000);
AL    Sgr |since JD2426000 - see Table.
AN    Sgr |P var. Max = 2425720 + 339.62d*E (JD2415000 - 26000);
AN    Sgr |Max = 2428360 + 330.0d*E (JD2426000 - 28500);
AN    Sgr |since JD2428500 - see Table.
AP    Sgr |SB? [09004].
AR    Sgr |There is a square term in the elements:
AR    Sgr |-[0.0031d (E-30)**2 + 8.8d].
AS    Sgr |Planetary nebula HB6 = 7 + 1deg 1.
AU    Sgr |In the region of the open cluster and the diffuse nebula
AU    Sgr |NGC 6514 (M20).
AV    Sgr |In the region of the open cluster NGC 6546. Not a member
AV    Sgr |of the cluster. [A/H] = 0.4. P var.
AV    Sgr |Max = 2429083.30 + 15.4093d*E (JD2421400 - 39100); since
AV    Sgr |JD2439100 - see Table.
AW    Sgr |VB A (B 16m, 15", 97deg).
AW    Sgr |In the region of the open cluster NGC 6546.
AY    Sgr |[A/H] = 0.2.
BB    Sgr |VB A (B = V4088 Sgr, 7.49m - 7.87m, 93.5", 102deg).
BB    Sgr |In the region of the open cluster Cr394.
BE    Sgr |A var (0.6m <= A <= 1.1m).
BM    Sgr |P var.
BN    Sgr |Min II 9.37; d = 0.04P:.
BN    Sgr |Soft X-ray source. P var [01600].
BQ    Sgr |d = 0.017P. P var. Min = 2412592.7905 + 8.01964d*E
BQ    Sgr |(JD2412590 - 22220) [01696]; since JD2422220 - see Table.
CC    Sgr |In the region of the globular cluster NGC 6723.
CD    Sgr |In the region of the globular cluster NGC 6723. P var.
CD    Sgr |Max = 2416247 + 266.62d*E
CD    Sgr |(JD2411000 - 23000); since JD2423000 - see Table.
CE    Sgr |In the region of the globular cluster NGC 6723.
CE    Sgr |SF component of a close double.
CF    Sgr |In the region of the globular cluster NGC 6723.
CF    Sgr |P var. Max = 2415632.81 + 0.570026d*E (JD2411000 -
CF    Sgr |23800) [01616]; since JD2423900 - see Table.
CG    Sgr |In the region of the globular cluster NGC 6723.
DH    Sgr |In the region of the globular cluster NGC 6809 (M55).
DI    Sgr |In the region of the globular cluster NGC 6809 (M55).
DK    Sgr |In the region of the globular cluster NGC 6809 (M55).
DM    Sgr |In the region of the globular cluster NGC 6809 (M55).
DO    Sgr |In the region of the globular cluster NGC 6809 (M55).
DP    Sgr |In the region of the globular cluster NGC 6809 (M55).
DR    Sgr |In the region of the globular cluster NGC 6809 (M55).
DS    Sgr |In the region of the globular cluster NGC 6809 (M55).
DV    Sgr |d = 0.044P.
EG    Sgr |d = 0.010P.
FV    Sgr |P var. Max = 2424010 + 269.5d*E (JD2424000 - 27500)
FV    Sgr |[00251]; since JD2427500 - see Table.
GG    Sgr |P var. Max = 2413840 + 286.5d*E (JD2413800 - 24000);
GG    Sgr |since JD2424000 - see Table.
GK    Sgr |According to [05869] - eclipsing.
GU    Sgr |There are also light variations with <P> = 37.5d,
GU    Sgr |0.4m <= A(V) <= 1.5m [06273].
HH    Sgr |VB (ro = 0.1').
IR    Sgr |VB B (A 13.6m; B 10", 220deg).
KO    Sgr |Similar to UG. It is possible that the observations in Min
KO    Sgr |brightness refer to a companion.
LZ    Sgr |VB A (B 16m, 7", 30deg).
MV    Sgr |Very hot hydrogen deficient extreme helium carbon star.
MW    Sgr |P var. Max = 2418940 + 202.3d*E (JD2418900 - 23900);
MW    Sgr |Max = 2428753 + 206.5d*E (JD2423900 - 28950);
MW    Sgr |since JD2428950 - see Table.
NP    Sgr |The cycles 100 - 300d are possible.
OW    Sgr |In the region of the open cluster NGC 6716.
V0348 Sgr |VB A (B 15m pg, 16", 73deg). Very hot hydrogen deficient
V0348 Sgr |helium carbon star.
V0348 Sgr |By the character of light variation and the spectrum the
V0348 Sgr |star is unique. The light curve resembling those of RCB
V0348 Sgr |type stars is superimposed by conspicuons irregular and
V0348 Sgr |semiregular variations with the mean cycle about 200d
V0348 Sgr |[02449,09824]. The star is surrounded by a nebula the
V0348 Sgr |radius of which equals 1". A fainter nebulous envelope is
V0348 Sgr |observed up to 7" from the star. Large infrared
V0348 Sgr |excess. Spectrum description [02451,09825]. Probably
V0348 Sgr |the star is intermediate between the RCB variables
V0348 Sgr |And planetary nebula Wolf-Rayet central stars.
V0350 Sgr |SB [09004].
V0354 Sgr |d = 0.02P.
V0356 Sgr |Min II 7.24; DII = 0.20P:; d = 0.05P;
V0356 Sgr |0.490P (1928) <= Min II - Min I <= 0.505P (1951).
V0356 Sgr |Apsidal motion is possible.
V0366 Sgr |P var. Max = 2425479.448 + 0.4779616d*E (JD2423990 - 28780)
V0366 Sgr |[00705]; since JD2435600 - see Table. [Ca/H] = -0.73.
V0367 Sgr |[Ca/H] = -1.21.
V0377 Sgr |The epoch of light min is given in the Table.
V0377 Sgr |P var. Min = 2426071.24 + 16.17076d*E (JD2425300 - 26600)
V0377 Sgr |[00048]; Min = 2427350.25 + 16.19326d*E (JD2426600 - 28700)
V0377 Sgr |[01400]; Min = 2436358.98 + 16.1575d*E
V0377 Sgr |(JD2436200 - 37300); Min = 2437863.09 + 16.1925d*E
V0377 Sgr |(JD2437660 - 39100); Min = 2440114.81 + 16.2407d*E
V0377 Sgr |(JD2440200 - 560); since JD2440950 - see Table.
V0397 Sgr |There is a square term in the elements:
V0397 Sgr |-0.009d*10**(-6)*E**2
V0401 Sgr |Min II 14.1.
V0403 Sgr |There is a nonlinear term in the elements:
V0403 Sgr |-0.013d*10**(-6)*E**2.
V0410 Sgr |VB A (B 13.6m, 270deg).
V0426 Sgr |Min II 13.3.
V0427 Sgr |There is a nonlinear term in the elements:
V0427 Sgr |-131d*10**(-10)*E**2. The shape of the light curve varies:
V0427 Sgr |0.17P <= M - m <= 0.22P.
V0431 Sgr |Min II 14.9.
V0437 Sgr |Min II 14.0.
V0440 Sgr |Delta(S) = 9. P var. P = 0.4774659d (JD2416000 - 23000)
V0440 Sgr |[00752]; P < 0.4774659d (JD2422000 - 26000) [00235];
V0440 Sgr |Max = 2426581.203 + 0.477474d*E (JD2426000 - 29460) [01000];
V0440 Sgr |since JD2437100 - see Table.
V0453 Sgr |There is a nonlinear term in the elements:
V0453 Sgr |+0.003d*10**(-6)*E**2.
V0457 Sgr |There is a nonlinear term in the elements:
V0457 Sgr |-0.005d*10**(-6)*E**2.
V0466 Sgr |There is a nonlinear term in the elements:
V0466 Sgr |+0.03d*10**(-6)*E**2.
V0496 Sgr |Min II 14.3.
V0497 Sgr |Min II 16.0.
V0505 Sgr |Min II 6.63. P var. Min I = 2433515.3295 + 1.18287141d*E
V0505 Sgr |(JD2425500 - 35800) [01642]; Min I = 2437494.4964 +
V0505 Sgr |1.1828622d*E (JD2435800 - 37500); Min I =
V0505 Sgr |2440055.3991 + 1.1828650d*E (JD2437500 - 40100);
V0505 Sgr |Min I = 2442656.5283 + 1.18286917d*E (JD2440100 -
V0505 Sgr |42670); since JD2442670 - see Table. The shape of the
V0505 Sgr |light curve varies. Deviations from the mean light curve
V0505 Sgr |vary with P = 310d. The difference of Min I and Min II
V0505 Sgr |depths varies by 0.05m [09830].
V0511 Sgr |P var. Max = 2423950 + 158.8d*E (JD2411300 - 23950);
V0511 Sgr |since JD2423950 - see Table.
V0515 Sgr |There is a nonlinear term in the elements: +0.015d*E**2.
V0519 Sgr |There is a nonlinear term in the elements: +0.0046d*E**2.
V0520 Sgr |There is a nonlinear term in the elements: +0.051d*E**2.
V0523 Sgr |Min II 9.88. Apsidal motion is observed. In the Table the
V0523 Sgr |epoch of Min I is given corresponding to the moment of
V0523 Sgr |line of apsides coinciding with the line of sight, when
V0523 Sgr |Min II - Min I = 0.50P. The mean period according to
V0523 Sgr |[02453] is given; with this period O - C deviations do not
V0523 Sgr |exceed  +-0.06P for both minima. The period of apsidal
V0523 Sgr |motion is 248 years [02453]. Min II - Min I = 0.39P in 1953.
V0524 Sgr |Min II 11.2.
V0525 Sgr |Min II 8.51.
V0526 Sgr |VB A (B 12.40m, 8.6", 7.3deg). Min II 10.20, DII = 0.17P;
V0526 Sgr |dI = 0.006P, dII = 0.013P.
V0526 Sgr |There are periodic terms in the elements:
V0526 Sgr |+0.1369d*sin(0.01295deg*E) - 0.0115d*sin(0.0259deg*E) +
V0526 Sgr |0.0011d*sin(0.0388deg*E). Min II = 2422055.0453 +
V0526 Sgr |1.919411d*E - 0.1369d*sin(0.01295deg*E) -
V0526 Sgr |0.0115d*sin(0.0259deg*E) - 0.0011d*sin(0.0388deg*E).
V0526 Sgr |The period of apsidal motion is 146 years. e = 0.224.
V0527 Sgr |P var. Max = 2426904.95 + 1.258956d*E (JD2425790 - 7650)
V0527 Sgr |[01648]; since JD2438200 - see Table.
V0551 Sgr |VB B (A 16.5m; B 12", 135deg).
V0552 Sgr |P var. The elements given in the Table are
V0552 Sgr |valid since JD2418400.
V0554 Sgr |Min II 14.5.
V0557 Sgr |P var. Max = 2415110.5 + 16.233d*E (JD2415100 - 22000);
V0557 Sgr |Max = 2426100.0 + 16.260d*E (JD2423900 - 27700) [00251];
V0557 Sgr |Max = 2428097.70 + 16.171d*E (JD2427700 - 28800) [00296];
V0557 Sgr |since JD2428800 - see Table.
V0558 Sgr |Min II 14.3.
V0564 Sgr |P var. Max = 2424056 + 27.8d*E (JD2423780 - 26000)
V0564 Sgr |[00251]; Max = 2428403.3 + 27.99d*E (JD2427870 - 29160)
V0564 Sgr |[00296]; Max = 2429158.2 + 27.2d (JD2429150 - 515);
V0564 Sgr |since JD2429515 - see Table.
V0567 Sgr |The central star of the planetary nebula P.K.355 -6deg 1
V0567 Sgr |(M3-21).
V0573 Sgr |Min II 12.7.
V0574 Sgr |Min II 14.7.
V0578 Sgr |According to [02448], Max = 2428710 + 253d*E.
V0593 Sgr |P var. Max = 2414150 + 230d*E (JD2414100 - 22900);
V0593 Sgr |since JD2423900 - see Table.
V0598 Sgr |d = 0.05P.
V0611 Sgr |P var. Max = 2414150 + 123d*E (JD2414150 - 19000);
V0611 Sgr |since JD2420250 - see Table.
V0611 Sgr |The period must probably be doubled because the star
V0611 Sgr |resembles RV Tau (Min II 16.2).
V0612 Sgr |P var. Max = 2413750 + 107.9d*E (JD2413700 - 17900);
V0612 Sgr |since JD2418800 - see Table.
V0615 Sgr |P.K.356 -7deg 1 = He 2-349.
V0626 Sgr |P var? Max = 2427715.4 + 26.745d*E (JD2425380 - 28800)
V0626 Sgr |[00046]; since JD2434500 - see Table.
V0631 Sgr |Min II 14.2.
V0632 Sgr |P var. Max = 2413350 + 263d*E (JD2413300 - 19000);
V0632 Sgr |since JD2420200 - see Table.
V0633 Sgr |P var. Max = 2415110 + 224d:*E (JD2415000 - 18800);
V0633 Sgr |since JD2420000 - see Table.
V0638 Sgr |P var? Max = 2412670 + 73.1d*E (JD2412600 - 14540);
V0638 Sgr |since JD2414800 - see Table.
V0646 Sgr |P var. Max = 2413350 + 95d*E (JD2413300 - 15900);
V0646 Sgr |since JD2423900 - see Table.
V0660 Sgr |P var. Max = 2426460 + 235.6d*E (JD2426400 - 35700)
V0660 Sgr |[00251]; since JD2435600 - see Table.
V0663 Sgr |P var. Max = 2426160 + 305d*E [00251];
V0663 Sgr |since JD2435600 - see Table.
V0671 Sgr |P = 292.5d?
V0672 Sgr |P var? Max = 2424680 + 228d*E [00251]; since
V0672 Sgr |JD2435600 - see Table.
V0674 Sgr |P var. Max = 2425830 + 249d*E [00251]; since
V0674 Sgr |JD2435600 - see Table.
V0675 Sgr |(k - b)2 = -0.01; Delta(S) = 11.
V0676 Sgr |P var. Max = 2414140 + 181d*E (JD2414100 - 22600)
V0676 Sgr |[00251]; since JD2423900 - see Table.
V0679 Sgr |P var. Max = 2415900 + 225d*E (JD2415900 - 22200)
V0679 Sgr |[00251]; Max = 2425440 + 223.1d*E (JD2425000 - 29000);
V0679 Sgr |since JD2429000 - see Table.
V0683 Sgr |Min II 12.5.
V0686 Sgr |P var? Max = 2425390 + 225.3d*E [00251]; since
V0686 Sgr |JD2435600 - see Table.
V0687 Sgr |Min II 12.2.
V0691 Sgr |P var? Max = 2426095.550 + 0.46911d*E [00251];
V0691 Sgr |since JD2435630 - see Table.
V0703 Sgr |Var 4. According to [02951] the range of light variation,
V0703 Sgr |the type of variability and the elements of light
V0703 Sgr |variation are erroneously assigned in [01640] to the star
V0703 Sgr |Var 3.
V0705 Sgr |Min II 12.9.
V0710 Sgr |P var. Min = 2426101.550 + 2.3817d*E [00251]; Min =
V0710 Sgr |2431286.425 + 2.381633d*E (JD2428390 - 35700) [03513].
V0713 Sgr |P var? Max = 2424680 + 253.4d*E [00251]; since
V0713 Sgr |JD2435600 - see Table.
V0716 Sgr |P var? Max = 2424670 + 277d*E [00251]; since
V0716 Sgr |JD2435600 - see Table.
V0718 Sgr |P var? Max = 2425850 + 153.2d*E [00251]; since
V0718 Sgr |JD2435600 - see Table.
V0721 Sgr |P = 71:d?
V0725 Sgr |Unique star.
V0725 Sgr |The mean brightness increased from 13.0m to 12.4m
V0725 Sgr |since 1889 to 1915, and fell to 12.8m in 1926. From
V0725 Sgr |1895 to 1926 real shortperiodic oscillations with the
V0725 Sgr |amplitude about 0.4m. In 1928 the amplitude suddenly
V0725 Sgr |increased by almost 2m, but the magnitude in maximum
V0725 Sgr |remained unchanged. From 1928 to 1935 the light
V0725 Sgr |variations became periodic, the period increasing every
V0725 Sgr |year by 1d in accordance with the formula:
V0725 Sgr |Min = 2426087 + 15.933d*E + 0.0233d*E**2.
V0725 Sgr |In 1935 P = 21d. Since 1936 only small oscillations of
V0725 Sgr |brightness with a gradual increase of the mean magnitude
V0725 Sgr |from 14.3m to 13.9m B (1969). Photoelectric observations
V0725 Sgr |in 1968 - 69 reveal the light variations 12.33m - 12.72m V
V0725 Sgr |with possible periods 15.4d in 1968 and 45.3d in 1969. In
V0725 Sgr |1973 12.28m - 12.58m V, <B-V> = +1.37, P = 50d [07101].
V0727 Sgr |VB A (B = V728 Sgr, 14.7m - 15.9m, 25", 108deg).
V0728 Sgr |VB B (A = V727 Sgr, B 25", 108deg).
V0734 Sgr |Min II 13.1.
V0735 Sgr |VB A (B 15.5m, 6", 315deg). According to B-V, U-B values
V0735 Sgr |and spectrum the star is not a UG type variable [09840].
V0738 Sgr |In the region of the globular cluster NGC 6558.
V0738 Sgr |According to [05403], RV? P = 86.78d?
V0743 Sgr |Min II 14.2.
V0745 Sgr |P var. Max = 2416560 + 385.1d*E (JD2411000 - 19260);
V0745 Sgr |since JD2419260 - see Table.
V0748 Sgr |Min II 14.7; d = 0.04P.
V0750 Sgr |d = 0.02P:.
V0752 Sgr |Min II 12.7.
V0755 Sgr |d = 0.01P.
V0757 Sgr |Min II 13.8; d = 0.06P.
V0760 Sgr |Min II 13.4. P var. Min = 2414059.5 + 45.10d*E
V0760 Sgr |(JD2412800 - 19000); since JD2419000 - see Table.
V0761 Sgr |Min II 12.8; d = 0.05P.
V0762 Sgr |P var. Max = 2414100 + 461d*E (JD2411000 - 22860);
V0762 Sgr |since JD2422860 - see Table.
V0763 Sgr |P var. The observations are satisfied by the given
V0763 Sgr |elements since JD2415000.
V0766 Sgr |d = 0.05P.
V0768 Sgr |Min II 13.0.
V0770 Sgr |Min II 13.1.
V0773 Sgr |[A/H] = 0.1.
V0777 Sgr |d = 0.055P.
V0778 Sgr |Min II 12.1.
V0779 Sgr |Min II 12.0.
V0780 Sgr |Min II 12.9; d = 0.08P.
V0782 Sgr |d = 0.045P.
V0784 Sgr |Min II 12.8.
V0786 Sgr |d = 0.025P.
V0789 Sgr |In the region of the open cluster Tr 31.
V0789 Sgr |P = 5.10470d (Min II 12.7)? [00478].
V0791 Sgr |d = 0.03P:.
V0792 Sgr |Min II 12.2. In the region of the open cluster
V0792 Sgr |and the diffuse nebula NGC 6514 (M 20).
V0793 Sgr |P var. Max = 2412610 + 195d*E (JD2412600 - 19400);
V0793 Sgr |since JD2423400 - see Table.
V0794 Sgr |P var. Min I = 2413723 + 173.48d*E (JD2413700 -
V0794 Sgr |23750); since JD2423750 - see Table.
V0801 Sgr |Min II 14.9.
V0802 Sgr |[A/H] = -0.4.
V0803 Sgr |P = 3.771748d?
V0818 Sgr |The shape of the light curve varies.
V0819 Sgr |P var?
V0824 Sgr |Min II 15.2.
V0828 Sgr |There is a close companion.
V0838 Sgr |P var?
V0839 Sgr |P var? Max = 2426170.126 + 1.835347d*E (JD2425700 - 26600)
V0839 Sgr |[01598]; since JD2441500 - see Table.
V0841 Sgr |The shape of the light curve varies.
V0844 Sgr |P var?
V0845 Sgr |Min II 14.6.
V0859 Sgr |The shape of the light curve varies.
V0879 Sgr |There is a close companion.
V0882 Sgr |Min II 14.6.
V0884 Sgr |0.20P <= M - m <= 0.40P. Blazhko effect.
V0889 Sgr |0.14P <= M - m <= 0.24P. Blazhko effect.
V0902 Sgr |Min II 14.8.
V0903 Sgr |Min II 13.0.
V0919 Sgr |Spectrum description [09845].
V0935 Sgr |P var. Max = 2420040 + 232.0d*E (JD2419500 - 28650);
V0935 Sgr |since JD2428600 - see Table.
V0938 Sgr |P = 138.27d?
V0960 Sgr |nP = 1734d.
V0966 Sgr |Min II 14.0.
V0977 Sgr |d = 0.03P.
V0981 Sgr |Min II 14.8.
V0985 Sgr |Min II 14.3.
V0986 Sgr |d = 0.015P.
V0993 Sgr |dI = 0.05P:; Min II 13.7, DII = 0.09P, dII = 0.00P.
V0994 Sgr |Min II 12.8:.
V0998 Sgr |The depth of Min II 0.04m:.
V1000 Sgr |Min II 13.9.
V1002 Sgr |Min II 13.7.
V1004 Sgr |[A/H] = -0.2.
V1005 Sgr |Min II 13.9.
V1013 Sgr |Min II 15.0.
V1017 Sgr |VB B (A 10.6m V; B 15", 270deg).
V1017 Sgr |For a long time the star was considered to be a recurrent
V1017 Sgr |nova. Three considerable flares were observed: in 1901
V1017 Sgr |(10.8m), 1919 (6.2m), and 1973 (10.5m). Composite spectrum
V1017 Sgr |with a trace of a hot component [03872].
V1023 Sgr |In the region of the open cluster Cr 394. Min II 13.0:.
V1026 Sgr |Min II 13.4.
V1028 Sgr |Min II 14.4.
V1032 Sgr |Min II 15.0.
V1033 Sgr |The shape of the light curve varies. Blazhko effect?
V1034 Sgr |d = 0.025P:.
V1049 Sgr |Min II 13.6; Min II - Min I = 0.326P; DII = 0.025P.
V1050 Sgr |Min II 14.1.
V1056 Sgr |Min II 14.1.
V1063 Sgr |The shape of the light curve strongly varies. Blazhko
V1063 Sgr |effect?
V1068 Sgr |Min II 15.4.
V1069 Sgr |The shape of the light curve strongly varies. Blazhko
V1069 Sgr |effect?
V1071 Sgr |P = 1.3560996d?
V1072 Sgr |The shape of the light curve strongly varies. Blazhko
V1072 Sgr |effect?
V1080 Sgr |P var. The shape of the light curve varies.
V1081 Sgr |P var?
V1089 Sgr |Cycle <= 30d.
V1100 Sgr |d = 0.02P:.
V1108 Sgr |Min II 11.9; Min II - Min I = 0.516P.
V1109 Sgr |Min II 14.5.
V1127 Sgr |There is a nonlinear term in the elements:
V1127 Sgr |+78.10d**(-10)*E**2.
V1136 Sgr |d = 0.020P.
V1148 Sgr |In the region of the globular cluster NGC 6553.
V1153 Sgr |P var? Max = 2428391.266 + 1.332624d*E (JD2427680 -
V1153 Sgr |30910); since JD2435630 - see Table.
V1177 Sgr |Min II 11.4.
V1178 Sgr |d = 0.03P:.
V1180 Sgr |[A/H] = -0.4.
V1181 Sgr |[A/H] = 0.6. P var. Max = 2428452.25 + 21.341d*E
V1181 Sgr |(JD2427400 - 31000) [01638]; since JD2433000 - see Table.
V1185 Sgr |[A/H] = -0.5. P var. Max = 2428778.86 + 13.9123d*E
V1185 Sgr |(JD2427500 - 32750) [01638]; Max = 2437485.4 +
V1185 Sgr |13.901345d*E (JD2437100 - 43760) [08519];
V1185 Sgr |since JD2444000 - see Table.
V1187 Sgr |[A/H] = -0.8.
V1188 Sgr |[CA/H] = -0.37.
V1189 Sgr |[A/H] = -1.1.
V1190 Sgr |P = 3.000078d?
V1191 Sgr |Min II 14.4.
V1205 Sgr |The alternative period is possible: 0.659820d [01638].
V1209 Sgr |A var.
V1211 Sgr |Delta(S) = 3:.
V1214 Sgr |There is a nonlinear term in the elements:
V1214 Sgr |-0.25d*10**(-7)*E**2.
V1216 Sgr |mu = 0.720", P = 106.7deg.
V1223 Sgr |As a rule has a persistent high state; five drops by two
V1223 Sgr |to more than three magnitudes have been registered and a
V1223 Sgr |twelve year interval of irregular variations at
V1223 Sgr |intermediate magnitudes. According to [09850] there are
V1223 Sgr |slow variations in brightness by 0.15m on a time scale
V1223 Sgr |of ~1 day. They are superimposed by variations with the
V1223 Sgr |orbital period P orb (Max = 2444749.9866 + 0.140239d*E)
V1223 Sgr |and with amplitude up to 0.15m. These variations in their
V1223 Sgr |turn are superimposed by the others: with P = 794.38s
V1223 Sgr |and the amplitude from 0.03m up to 0.15m
V1223 Sgr |(Max = 2444750.00404 + 0.009194215d*E and (sometimes) with
V1223 Sgr |P = 849.8s and a twice smaller amplitude
V1223 Sgr |(Max = 2444750.00350 + 0.00983588d*E). Besides there are
V1223 Sgr |rapid brightness variations on time scales 10 - 100s by
V1223 Sgr |0.10m - 0.20m, and high frequency flickering by 0.05m.
V1223 Sgr |According to [09851], the period of X-ray pulses associated
V1223 Sgr |with the rotation of the compact object is 12.5 minutes.
V1276 Sgr |Min II 14.3.
V1280 Sgr |Brightness of Max varies by 2m with the period 5230d.
V1281 Sgr |The light variation is not strictly periodic.
V1282 Sgr |P var. Min = 2427651.297 + 1.754574d*E (JD2427650 -
V1282 Sgr |30560) [00705]; since JD2435600 - see Table.
V1284 Sgr |Min II 13.5. EB?
V1287 Sgr |Var 3. According to [02951] the range of light variation of
V1287 Sgr |Var 4 (V703 Sgr), the type of variability and the elements
V1287 Sgr |of light variation of Var 4 (V703) are erroneously
V1287 Sgr |assigned in [01640] to the star Var 3.
V1287 Sgr |According to [02951] the range of light variation, the type
V1287 Sgr |of variability and the elements of light variation are
V1287 Sgr |erroneously assigned in [01640] to the star Var 4.
V1287 Sgr |Min II 14.8.
V1290 Sgr |[A/H] = -1.2.
V1303 Sgr |[A/H] = -0.8. P var? Max = 2438241.176 + 18.46812d*E
V1303 Sgr |(JD2427700 - 38250) [00001]; since JD2444000 - see Table.
V1304 Sgr |[A/H] = 0.3. P var. Max = 2428758.10 + 12.9287d*E
V1304 Sgr |(JD2427590 - 28820) [01640]; since JD2435600 - see Table.
V1309 Sgr |Not far from V4032 Sgr.
V1311 Sgr |V 14 in the globular cluster NGC 6656 (M22).
V1311 Sgr |Not a member of the cluster.
V1312 Sgr |P var? Max = 2428815.600 + 0.6011427d*E (JD2427590 - 28820)
V1312 Sgr |[01640]; since JD2435630 - see Table.
V1314 Sgr |P var? Max = 2428346.536 + 0.657489d*E (JD2427600 -
V1314 Sgr |28820) [01640]; since JD2435630 - see Table.
V1317 Sgr |P var?
V1327 Sgr |SR?, L? [08424].
V1328 Sgr |P = 0.39937d?
V1329 Sgr |VB B (A 17.2m; B 1.4", 120deg). P var. Max = 2432388.777 +
V1329 Sgr |0.48306d*E (JD2431670 - 32740) [03524];
V1329 Sgr |since JD2443300 - see Table.
V1331 Sgr |Min II 16.5.
V1352 Sgr |P var. Max = 2431998.851 + 0.49505d*E (JD2431670 -
V1352 Sgr |33150) [01680]; Max = 2443341.844 + 0.49493d*E
V1352 Sgr |(JD2443300 - 350); Max = 2444087.558 + 0.49516d*E
V1352 Sgr |(JD2444050 - 110); in the interval JD2444400 - 410 - see
V1352 Sgr |Table.
V1356 Sgr |Min II 18.0:.
V1357 Sgr |Min II 19.0.
V1359 Sgr |P var?
V1369 Sgr |P var. Max = 2432736.821 + 0.52956d*E (JD2431670 - 33150)
V1369 Sgr |[03524]; since JD2440700 - see Table.
V1374 Sgr |Delta(S) = 1.
V1378 Sgr |Delta(S) = -3:.
V1387 Sgr |Delta(S) = 3.
V1389 Sgr |The epoch of Min brightness is given.
V1390 Sgr |Min II 17.6.
V1392 Sgr |P var. Max = 2432739.791 + 0.55032d*E (JD2431670 - 33150)
V1392 Sgr |[03524]; since JD2440700 - see Table.
V1393 Sgr |Delta(S) = 3.
V1394 Sgr |Min II 18.0.
V1401 Sgr |The epoch of Min brightness is given.
V1405 Sgr |P var. Max = 2432031.778 + 0.46511d*E (JD2431670 - 33150)
V1405 Sgr |[06094]; since JD2443300 - see Table.
V1408 Sgr |A var (0.5m <= A <= 1.4m).
V1409 Sgr |P var. Max = 2432739.822 + 0.65159d*E (JD2431670 - 33150)
V1409 Sgr |[03524]; since JD2443300 - see Table.
V1412 Sgr |The epoch of Min brightness is given.
V1415 Sgr |P var?
V1416 Sgr |Delta(S) = 3. P var? Max = 2432002.875 + 0.42767d*E
V1416 Sgr |(JD2431670 - 33150) [06094]; since JD2440700 - see Table.
V1418 Sgr |P var. Max = 2432740.818 + 0.45423d*E (JD2431670 - 33150)
V1418 Sgr |[03524]; since JD2440700 - see Table.
V1419 Sgr |P var. Max = 2432061.669 + 0.57144d*E (JD2431670 - 33150)
V1419 Sgr |[01680]; since JD2440700 - see Table.
V1425 Sgr |Min II 18.8.
V1426 Sgr |Delta(S) = 1.5.
V1429 Sgr |The epoch of Min brightness is given.
V1435 Sgr |Min II 18.0; Min II - Min I = 0.53P.
V1437 Sgr |V8 (NGC 6522); not a member of the globular cluster.
V1438 Sgr |V9 (NGC 6522); not a member of the globular cluster.
V1439 Sgr |P = 0.53711d? [06094].
V1443 Sgr |Min II 18.6.
V1446 Sgr |Min II 18.0.
V1447 Sgr |Min II 18.2.
V1454 Sgr |Min II 15.4.
V1457 Sgr |Min II 19.0.
V1459 Sgr |The depth of Min II is 0.04m.
V1460 Sgr |P var. Max = 2432067 + 162.0d*E (JD2431670 - 33150)
V1460 Sgr |[01680]; since JD2440340 - see Table.
V1464 Sgr |Delta(S) = 1.
V1465 Sgr |P var. Max = 2431702.660 + 0.45757d*E (JD2431700 - 940);
V1465 Sgr |Max = 2432706.945 + 0.45757d*E (JD2431940 - 32740) [03524];
V1465 Sgr |since JD2440740 - see Table.
V1466 Sgr |The epoch of Min brightness is given.
V1473 Sgr |According to [08424] P = 340d.
V1487 Sgr |Min II 18.8.
V1491 Sgr |Min II 18.5.
V1498 Sgr |SP component of a close pair. P var.
V1498 Sgr |Max = 2432739.728 + 0.47467d*E (JD2431670 - 33150) [06094];
V1498 Sgr |since JD2443300 - see Table.
V1508 Sgr |VB.
V1509 Sgr |Min II 18.1:.
V1510 Sgr |According to [06094], P = 0.48546d.
V1516 Sgr |P var? Max = 2432740.753 + 0.49709d*E (JD2431670 -
V1516 Sgr |33150) [03524]; since JD2440700 - see Table.
V1517 Sgr |P < 2.0d.
V1523 Sgr |P var? Max = 2432417.702 + 0.36202d*E (JD2431670 - 33150)
V1523 Sgr |[03524]; since JD2443300 - see Table.
V1526 Sgr |Min II 18.3.
V1537 Sgr |Min II 17.4; Min II - Min I = 0.54P.
V1540 Sgr |According to [08424], P = 465d.
V1546 Sgr |The epoch of Min brightness is given.
V1550 Sgr |P = 0.37432d? [06094].
V1554 Sgr |Min II 17.5.
V1557 Sgr |Delta(S) = 8.
V1558 Sgr |Delta(S) = 1.
V1559 Sgr |The depth of MinII is 0.04m.
V1561 Sgr |Min II 17.7.
V1567 Sgr |Min II 18.0.
V1569 Sgr |Min II 18.6.
V1576 Sgr |[Ca/H] = -1.23.
V1577 Sgr |P var. Max = 2426200 + 290d*E (JD2426000 - 30560)
V1577 Sgr |[02449]; since JD2430560 - see Table.
V1580 Sgr |P var (310d <= P <= 365d).
V1589 Sgr |[Ca/H] = -0.91.
V1602 Sgr |d = 0.03P.
V1610 Sgr |P < 0.5d.
V1639 Sgr |The shape of the light curve varies.
V1640 Sgr |(k -b)2 = 0.24. P var?
V1642 Sgr |250d <= P <= 350d.
V1643 Sgr |Min II 12.1. According to [05771], RR?, P = 0.34d.
V1644 Sgr |The shape of the light curve varies.
V1647 Sgr |VB A (B 9.13m, 8", 104deg). Min II 7.43, DII = 0.059P,
V1647 Sgr |Min II - Min I = 0.262P (JD2441830);
V1647 Sgr |Min II = 2441830.55561 + 3.28282227d*E.
V1647 Sgr |The apsidal motion period is 592.5 +- 6.5 years.
V1648 Sgr |Close VB. Flat Min.
V1652 Sgr |Close VB. Flat Min.
V1653 Sgr |Close VB. Flat Min.
V1656 Sgr |Close VB. Flat Min.
V1658 Sgr |P var.Max = 2426560 + 105d*E (JD2417000 - 28000)
V1658 Sgr |[00842]; since JD2428000 - see Table.
V1660 Sgr |Close VB. Flat Min.
V1661 Sgr |Close VB. Flat Min. P var. Max = 2426850 + 275d*E
V1661 Sgr |(JD2424000 - 26850); since JD2436700 - see Table.
V1667 Sgr |P var. Max = 2426560 + 158d*E (JD2417000 - 36000)
V1667 Sgr |[00842]; since JD2436000 - see Table.
V1668 Sgr |Close VB. Flat Min.
V1670 Sgr |A var. P var. The shape of the light curve varies
V1670 Sgr |(probably with a period of about 11 years).
V1675 Sgr |A possible companion of 16m.
V1679 Sgr |Close VB. Flat Min.
V1681 Sgr |A possible companion of 16m.
V1690 Sgr |A possible companion of 16m.
V1691 Sgr |Close VB. Flat Min.
V1691 Sgr |P var. Max = 2426520 + 235d*E (JD2417000 - 28000)
V1691 Sgr |[00842]; since JD2436000 - see Table.
V1697 Sgr |A possible companion of 16m.
V1698 Sgr |A possible companion of 16m.
V1699 Sgr |P var. Max = 2425410 + 203.6d*E (JD2417000 - 27600)
V1699 Sgr |[00842]; since JD2436000 - see Table.
V1703 Sgr |A possible companion of 16m.
V1705 Sgr |P var. Max = 2425860 + 142d*E (JD2417000 - 27000)
V1705 Sgr |[00842]; since JD2435800 - see Table.
V1711 Sgr |[A/H] = -1.1. P var. Max = 2435365.19 + 30.46d*E
V1711 Sgr |(JD2432700 - 35400) [02570]; since JD2442200 - see Table.
V1714 Sgr |In the region of the open cluster Ruprecht 134.
V1721 Sgr |d = 0.03P:.
V1723 Sgr |Min II 13.8.
V1730 Sgr |Min II 14.8:; d = 0.03P:.
V1741 Sgr |In the nebula and the cluster NGC 6530 (M8). Var1.
V1743 Sgr |In the nebula and the cluster NGC 6530 (M8). Var2.
V1747 Sgr |In the nebula and the cluster NGC 6530 (M8). Var3.
V1748 Sgr |In the nebula and the cluster NGC 6530 (M8). Var4.
V1749 Sgr |In the nebula and the cluster NGC 6530 (M8). Var6.
V1750 Sgr |In the nebula and the cluster NGC 6530 (M8). Var8.
V1751 Sgr |In the nebula and the cluster NGC 6530 (M8). Var7.
V1752 Sgr |In the nebula and the cluster NGC 6530 (M8). Var13.
V1753 Sgr |In the nebula and the cluster NGC 6530 (M8). Var14.
V1755 Sgr |In the nebula and the cluster NGC 6530 (M8). Var15.
V1758 Sgr |In the nebula and the cluster NGC 6530 (M8). Var16.
V1761 Sgr |In the nebula and the cluster NGC 6530 (M8). Var19.
V1762 Sgr |In the nebula and the cluster NGC 6530 (M8). Var20.
V1764 Sgr |In the nebula and the cluster NGC 6530 (M8). Var23.
V1765 Sgr |In the nebula and the cluster NGC 6530 (M8). Var24.
V1768 Sgr |In the nebula and the cluster NGC 6530 (M8). Var26.
V1769 Sgr |In the nebula and the cluster NGC 6530 (M8). Var27.
V1771 Sgr |In the nebula and the cluster NGC 6530 (M8). Var29.
V1772 Sgr |In the nebula and the cluster NGC 6530 (M8). Var28.
V1773 Sgr |In the nebula and the cluster NGC 6530 (M8). Var31.
V1774 Sgr |In the nebula and the cluster NGC 6530 (M8). Var30.
V1775 Sgr |In the nebula and the cluster NGC 6530 (M8). Var33.
V1776 Sgr |In the nebula and the cluster NGC 6530 (M8). Var36.
V1777 Sgr |In the nebula and the cluster NGC 6530 (M8). Var37.
V1778 Sgr |In the nebula and the cluster NGC 6530 (M8). Var34.
V1779 Sgr |In the nebula and the cluster NGC 6530 (M8). Var40.
V1780 Sgr |In the nebula and the cluster NGC 6530 (M8). Var39.
V1781 Sgr |In the nebula and the cluster NGC 6530 (M8). Var41.
V1782 Sgr |In the nebula and the cluster NGC 6530 (M8). Var44.
V1784 Sgr |In the nebula and the cluster NGC 6530 (M8). Var45.
V1785 Sgr |In the nebula and the cluster NGC 6530 (M8). Var46.
V1786 Sgr |In the nebula and the cluster NGC 6530 (M8). Var48.
V1787 Sgr |In the nebula and the cluster NGC 6530 (M8). Var47.
V1788 Sgr |In the nebula and the cluster NGC 6530 (M8). Var50.
V1789 Sgr |In the nebula and the cluster NGC 6530 (M8). Var51.
V1790 Sgr |In the nebula and the cluster NGC 6530 (M8). Var49.
V1790 Sgr |Western component of a close pair.
V1791 Sgr |In the nebula and the cluster NGC 6530 (M8). Var53.
V1792 Sgr |In the nebula and the cluster NGC 6530 (M8). Var55.
V1793 Sgr |In the nebula and the cluster NGC 6530 (M8). Var54.
V1794 Sgr |In the nebula and the cluster NGC 6530 (M8). Var56.
V1795 Sgr |In the nebula and the cluster NGC 6530 (M8). Var58.
V1797 Sgr |In the nebula and the cluster NGC 6530 (M8). Var59.
V1798 Sgr |In the nebula and the cluster NGC 6530 (M8). Var60.
V1800 Sgr |In the nebula and the cluster NGC 6530 (M8). Var61.
V1801 Sgr |In the nebula and the cluster NGC 6530 (M8). Var62.
V1802 Sgr |In the nebula and the cluster NGC 6530 (M8). Var63.
V1803 Sgr |In the nebula and the cluster NGC 6530 (M8). Var64.
V1803 Sgr |SP component of a close pair.
V1805 Sgr |In the nebula and the cluster NGC 6530 (M8). Var66.
V1807 Sgr |In the nebula and the cluster NGC 6530 (M8). Var67.
V1808 Sgr |In the nebula and the cluster NGC 6530 (M8). Var68.
V1828 Sgr |P var. Max = 2424402 + 12.985d*E (JD2423800 - 36000)
V1828 Sgr |[02515]; since JD2436000 - see Table.
V1831 Sgr |P var. Max = 2428849.4 + 26.58d*E (JD2427500 - 31270)
V1831 Sgr |[02447]; since JD2435630 - see Table.
V1843 Sgr |P = 163.7d? [05869].
V1845 Sgr |Flat Min. Close companion?
V1864 Sgr |Epoch of light maximum is given.
V1869 Sgr |P var. Max = 2434178 + 346d*E (JD2427590 - 34220)
V1869 Sgr |[02447]; since JD2435630 - see Table.
V1882 Sgr |The shape of the light curve varies.
V1891 Sgr |A companion of 16m.
V1894 Sgr |V4 (NGC 6637). Possible member of the globular cluster
V1894 Sgr |NGC 6637 (M 69).
V1895 Sgr |P var. Max = 2421065 + 156.0d*E (JD2418850 - 21100);
V1895 Sgr |since JD2427600 - see Table.
V1900 Sgr |A companion of 15m.
V1904 Sgr |A companion of 15m.
V1911 Sgr |P var. Max = 2428832.4 + 10.0581d*E (JD2427600 - 34220)
V1911 Sgr |[02447]; since JD2435630 - see Table. The shape of the
V1911 Sgr |light curve varies?
V1925 Sgr |P var?
V1942 Sgr |In the region of the open cluster Ruprecht 147.
V1945 Sgr |In the region of the open cluster and the diffuse nebula
V1945 Sgr |NGC 6514 (M20).
V1946 Sgr |In the region of the open cluster and the diffuse nebula
V1946 Sgr |NGC 6514 (M20).
V1947 Sgr |In the region of the open cluster and the diffuse nebula
V1947 Sgr |NGC 6514 (M20). All the published charts
V1947 Sgr |for this variable are wrong. According to [09861] the
V1947 Sgr |star actually lies 1.1 mm south and 0.8 mm east of
V1947 Sgr |"D2" in fugure 3 published in [02428].
V1948 Sgr |In the region of the open cluster and the diffuse nebula
V1948 Sgr |NGC 6514 (M20).
V1949 Sgr |In the region of the open cluster and the diffuse nebula
V1949 Sgr |NGC 6514 (M20).
V1950 Sgr |In the region of the open cluster and the diffuse nebula
V1950 Sgr |NGC 6514 (M20).
V1951 Sgr |In the region of the open cluster and the diffuse nebula
V1951 Sgr |NGC 6514 (M20).
V1954 Sgr |VB(ro = 2"). P var.
V1954 Sgr |There is a nonlinear term in the elements:
V1954 Sgr |-4.1313d*10**(-8)*E**2.
V1958 Sgr |Min II 14.0.
V1962 Sgr |In the region of the open cluster and the
V1962 Sgr |diffuse nebula NGC 6618 (M 17).
V1963 Sgr |In the region of the open cluster and the diffuse nebula
V1963 Sgr |NGC 6618 (M 17).
V1966 Sgr |In the region of the open cluster and the diffuse nebula
V1966 Sgr |NGC 6618 (M 17).
V1969 Sgr |There are three close faint companions (15.8m-16.3m).
V1970 Sgr |In the region of the open cluster and the diffuse nebula
V1970 Sgr |NGC 6618 (M 17).
V1971 Sgr |In the region of the open cluster and the diffuse nebula
V1971 Sgr |NGC 6618 (M 17).
V1973 Sgr |In the region of the open cluster and the diffuse nebula
V1973 Sgr |NGC 6618 (M 17).
V1975 Sgr |In the region of the open cluster and the diffuse nebula
V1975 Sgr |NGC 6618 (M 17). The presence of a blue companion is
V1975 Sgr |possible.
V1976 Sgr |In the region of the open cluster and the diffuse nebula
V1976 Sgr |NGC 6618 (M 17).
V1977 Sgr |In the region of the open cluster and the diffuse nebula
V1977 Sgr |NGC 6618 (M 17).
V1980 Sgr |Min II 11.7; DII = 0.11P; Min II - Min I = 0.52P.
V1996 Sgr |VB.
V2003 Sgr |S 5.5/5. In the region of the open cluster M 25 (IC 4725).
V2007 Sgr |V 26 (NGC 6656 = M 22).
V2008 Sgr |P = 120 - 135d.
V2028 Sgr |In the region of the globular cluster NGC 6681 (M 70).
V2037 Sgr |A close companion is possible.
V2054 Sgr |P > 450d?
V2064 Sgr |VB. Combined brightness of the star and the close
V2064 Sgr |companion was estimated. It is not clear which star is
V2064 Sgr |variable.
V2065 Sgr |NP component of a close binary.
V2094 Sgr |P < 0.5d.
V2106 Sgr |VB. Combined brightness of the components was estimated.
V2148 Sgr |VB. Combined brightness of the components was estimated.
V2148 Sgr |The variable is the northern component.
V2276 Sgr |P < 30d.
V2282 Sgr |Star L. In the region of the open cluster and the diffuse
V2282 Sgr |nebula NGC 6514 (M20). Late spectrum.
V2283 Sgr |Min II 10.59:. Apsidal motion with P = 560 years [07107]:
V2283 Sgr |0.739P (1898) <= Min II - Min I <= 0.797P (1965).
V2283 Sgr |There are periodic terms in the
V2283 Sgr |elements given in the Table:
V2283 Sgr |+0.5414d*sin(0.006deg*(E + 45019)) - 0.0995d*sin(0.012deg*
V2283 Sgr |(E + 45019)) + 0.0217d*sin(0.018deg*(E + 45019)); Min II =
V2283 Sgr |2438946.7619 + 3.4714231d*E - 0.5414d*sin(0.006deg*
V2283 Sgr |(E + 45019)) - 0.0995d*sin(0.012deg*(E + 45019)) - 0.0217d*
V2283 Sgr |sin(0.018deg*(E + 45019)).
V2284 Sgr |P var.
V2285 Sgr |In the region of the globular cluster NGC 6558.
V2313 Sgr |Min II 16.8.
V2315 Sgr |P = 0.193d?
V2323 Sgr |Blue [08424].
V2341 Sgr |The epoch of Min brightness is given.
V2342 Sgr |V 17 (NGC 6626 = M28).
V2342 Sgr |The member of this globular cluster. Min II 13.5.
V2343 Sgr |A close companion of 14.5m.
V2346 Sgr |Cycles 50 - 100d.
V2349 Sgr |Min II 9.2.
V2351 Sgr |Min II 10.31.
V2352 Sgr |P var. There is a nonlinear term in the elements:
V2352 Sgr |0.0525d*E**2.
V2355 Sgr |In the region of the globular cluster NGC 6637 (M 69).
V2358 Sgr |In the region of the globular cluster NGC 6642.
V2359 Sgr |In the region of the globular cluster NGC 6637 (M 69).
V2360 Sgr |In the region of the globular cluster NGC 6637 (M 69).
V2361 Sgr |In the region of the globular cluster NGC 6637 (M 69).
V2362 Sgr |A close companion of 15m.
V2366 Sgr |P var. There is a nonlinear term in the elements:
V2366 Sgr |+0.6815d*10**(-9)*E**2.
V2367 Sgr |V28 (NGC 6656 = M22). Not a member of this globular cluster.
V2367 Sgr |P = 323d?
V2378 Sgr |Two close companions of 15.3m and 15.8m.
V2389 Sgr |P var?
V2391 Sgr |P = 189d?
V2413 Sgr |P var. The elements are valid in the interval
V2413 Sgr |JD2425440 - 30905.
V2416 Sgr |P.K. 7 +1G 2.
V2425 Sgr |E?
V2442 Sgr |P = 0.5d?
V2449 Sgr |Min II 17.4.
V2468 Sgr |Blue [08424].
V2471 Sgr |VB B (A 14.6m; B 8", 225deg).
V2493 Sgr |Blue [08424].
V2506 Sgr |P.K. 3 -4deg 6.
V2507 Sgr |Min II 14.6.
V2508 Sgr |Min II 14.1:.
V2509 Sgr |Min II 7.50.
V2510 Sgr |The epoch of Min brigtness is given. The elements given
V2510 Sgr |in the Table are valid since JD2427440.
V2520 Sgr |VB.
V2526 Sgr |The epoch of Min brightness is given.
V2526 Sgr |P var. Min = 2428699.5 + 31.3224d*E (JD2424100 - 31400)
V2526 Sgr |[05590]. Since JD2431400 - see Table.
V2529 Sgr |Min II 14.5. Twice shorter period is given in [05590].
V2540 Sgr |P var.
V2544 Sgr |VB?
V2552 Sgr |VB A (B 15.7m).
V2553 Sgr |There are two close companions.
V2562 Sgr |Northern component of a close pair. The companion is of
V2562 Sgr |16m.
V2563 Sgr |P var.
V2564 Sgr |P var?
V2565 Sgr |VB B (A 12.5m; B 90deg).
V2566 Sgr |P var. [Ca/H] = -0.52.
V2567 Sgr |[Ca/H] = -0.57.
V2568 Sgr |P var?
V2576 Sgr |P var. Max = 2426200 + 149d*E (JD2423500 - 27000);
V2576 Sgr |since JD2433000 - see Table.
V2577 Sgr |P var?
V2578 Sgr |VB. In the region of the globular cluster NGC 6642.
V2579 Sgr |P var. Max = 2429926.251 + 0.5911903d*E (JD2427590 -
V2579 Sgr |34200) [05590]; since JD2435600 - see Table.
V2584 Sgr |P var. Max = 2426564.347 + 0.534829d*E (JD2423940 -
V2584 Sgr |33860); since JD2437820 - see Table.
V2592 Sgr |In the region of the globular cluster NGC 6656 (M22).
V2593 Sgr |P var. Max = 2428780.349 + 0.5123825d*E
V2593 Sgr |(JD2427680 - 34200) [05590]; since JD2435600 - see Table.
V2594 Sgr |P var.
V2598 Sgr |A companion 15.8m. Spectrum description [06495].
V2601 Sgr |P.K. 12 -7deg 1.  The epoch of Min brightness is given.
V2616 Sgr |Min II 13.0.
V2617 Sgr |Min II 9.63.
V2620 Sgr |P = 185.6d?
V2625 Sgr |P = 0.75837d?
V2628 Sgr |P = 171d:?/205d:?/256d:?.
V2645 Sgr |P var?
V2649 Sgr |P = 143d:?
V2672 Sgr |P = 196.8d? /204.5d, /255.3d? /315.0d?
V2682 Sgr |P = 228.5d?
V2687 Sgr |P = 174d:?
V2703 Sgr |P = 270d:?
V2719 Sgr |SR?
V2731 Sgr |P = 147d:?
V2732 Sgr |P = 188.6d?
V2733 Sgr |P = 244d:?
V2736 Sgr |[Ca/H] = -1.45.
V2738 Sgr |[Ca/H] = -0.67.
V2740 Sgr |P = 269.0d?
V2745 Sgr |[Ca/H] = -1.15.
V2756 Sgr |P.K. 2 -5deg 1. The epoch of Min brightness is given.
V2763 Sgr |P = 216d:?
V2777 Sgr |[Ca/H] = -0.83.
V2783 Sgr |P = 265.0d?
V2789 Sgr |P = 255.5d?
V2798 Sgr |P = 244.5d?
V2816 Sgr |P = 250d:?
V2828 Sgr |P = 0.39669d?
V2830 Sgr |Cepheid?
V2833 Sgr |P = 224.0d?
V2834 Sgr |P = 275d:?
V2846 Sgr |P = 0.39659d?
V2868 Sgr |P = 235.5d?
V2876 Sgr |Min II 15.7:.
V2877 Sgr |P = 254.5d?
V2893 Sgr |P = 250d:?
V2900 Sgr |P = 0.49835d?
V2905 Sgr |Spectrum description [04452,06495].
V2918 Sgr |P = 197d:?
V2937 Sgr |[Ca/H] = -0.75.
V2947 Sgr |RV Tau? Cepheid?
V2959 Sgr |P = 0.37233d?
V2962 Sgr |P = 209.5d?
V2967 Sgr |P = 0.68750d?
V2988 Sgr |P = 213.0d? The coordinates given in [05869] are erroneous.
V2996 Sgr |RV Tau? Cepheid?
V3004 Sgr |[Ca/H] = -0.76.
V3005 Sgr |RV Tau? Cepheid?
V3016 Sgr |P var?
V3032 Sgr |P = 153d:?
V3033 Sgr |The coordinates given in [05869] are erroneous.
V3034 Sgr |P = 154d:?
V3038 Sgr |P = 252d:?
V3052 Sgr |RV Tau? Cepheid?
V3062 Sgr |EW? P = 0.59610d?
V3065 Sgr |P = 179.8d?/215.5d?
V3071 Sgr |P = 291d:?
V3072 Sgr |P = 194d:?
V3088 Sgr |P = 215d:?
V3105 Sgr |[Ca/H] = -0.82.
V3106 Sgr |P = 261d:?
V3111 Sgr |P = 182.8d?
V3127 Sgr |UG? Not red.
V3128 Sgr |Nova? Only one Max was observed.
V3170 Sgr |[Ca/H] = -0.82.
V3175 Sgr |P = 179.8d?
V3176 Sgr |P = 197d:?
V3179 Sgr |P = 297d:?
V3186 Sgr |[Ca/H] = -1.28.
V3190 Sgr |P = 227.0d?
V3196 Sgr |RV Tau? Cepheid?
V3207 Sgr |P = 237d:?
V3239 Sgr |P = 226d:?
V3249 Sgr |UG?
V3285 Sgr |P = 173.8d /196.2d?
V3294 Sgr |P = 121d:? /177d:?
V3295 Sgr |P = 197d:?
V3335 Sgr |RV Tau? Cepheid?
V3353 Sgr |P var?
V3356 Sgr |P = 239.5d?
V3365 Sgr |P = 197d:? /252d:?
V3388 Sgr |P = 125d:? /160d:?
V3395 Sgr |P = 159d:?
V3412 Sgr |Cepheid?
V3433 Sgr |P = 287.0d?
V3443 Sgr |P = 177.6d?
V3444 Sgr |P = 160d:?
V3459 Sgr |P var. The shape of the light curve varies.
V3467 Sgr |RV Tau? Cepheid?
V3473 Sgr |SR?
V3500 Sgr |RV Tau? Cepheid?
V3501 Sgr |Min II 15.7:.
V3508 Sgr |The member of the open cluster M25 (IC 4725).
V3511 Sgr |RV Tau? Cepheid?
V3536 Sgr |P = 239.5d?
V3537 Sgr |P = 318.0d?
V3551 Sgr |P = 165.2d? /201.0d?
V3560 Sgr |P = 181d:?
V3564 Sgr |Cepheid?
V3566 Sgr |P = 249.0d?
V3583 Sgr |P = 228.0d?
V3588 Sgr |[Ca/H] = -0.69.
V3625 Sgr |P = 294d:?
V3634 Sgr |P = 145d:?
V3645 Sgr |In the region of the open cluster M25 (IC 4725).
V3709 Sgr |P = 240.0d?
V3718 Sgr |P var. There is a nonlinear term
V3718 Sgr |in the elements: +0.865d*10**(-10)*E**2.
V3748 Sgr |P = 0.305327d?
V3765 Sgr |[Ca/H] = -0.78.
V3783 Sgr |In the region of the globular cluster NGC 6681 (M70).
V3784 Sgr |P = 176.4d?
V3788 Sgr |In the region of the globular cluster NGC 6723. Red.
V3791 Sgr |In the region of the open cluster and the diffuse nebula
V3791 Sgr |NGC 6514 (M20).
V3792 Sgr |VB A (B 8.92m, 13.3", 90deg). Min II 6.81.
V3792 Sgr |The range of the combined light variation is given in the
V3792 Sgr |Table. The shape of the light curve varies.
V3804 Sgr |Spectrum description [06495,07099].
V3811 Sgr |P2 = 4d? Spectrum description [07099,09845].
V3817 Sgr |VB A (B 16m).
V3819 Sgr |P var. There is a nonlinear term in the elements:
V3819 Sgr |+10**(-10)*E**2.
V3829 Sgr |A close companion.
V3832 Sgr |A close companion.
V3834 Sgr |Cepheid or eclipsing?
V3837 Sgr |P = 0.565d? [06383].
V3838 Sgr |VB A (B 15.8m).
V3841 Sgr |P var. Max = 2431970 + 358d*E (JD2423900 - 33000);
V3841 Sgr |since JD2433000 - see Table.
V3842 Sgr |A close companion with M2? Spectral class possibly exists.
V3843 Sgr |In the region of the globular cluster NGC 6642.
V3853 Sgr |V22 (NGC 6656 = M22). The member of this globular cluster.
V3855 Sgr |V31 (NGC 6656 = M22). Possible member of the cluster.
V3857 Sgr |According to [06278] the spectral class is M8.
V3867 Sgr |Under the chart S 4903 is printed erroneously instead of
V3867 Sgr |CSV 4309.
V3868 Sgr |P var. Max = 2426130 + 270d*E (JD2423900 - 33900);
V3868 Sgr |since JD2435700 - see Table.
V3874 Sgr |P var. Max = 2436035 + 115.3d*E (JD2426000 - 38000);
V3874 Sgr |since JD2438000 - see Table.
V3875 Sgr |P var. P = 358d (JD2424000 - 33800); since
V3875 Sgr |JD2435000 - see Table.
V3876 Sgr |P var. Max = 2430090 + 345d*E (JD2423900 - 32000);
V3876 Sgr |Max = 2436830 + 358d*E (JD2436000 - 41500) [06279];
V3876 Sgr |since JD2441400 - see Table.
V3879 Sgr |VB (Delta(m) = 2.6m, ro = 0.6").
V3880 Sgr |OH, SiO, H2O maser.
V3885 Sgr |Porb = 0.206d [04939].
V3885 Sgr |Besides the irregular variability high-frequency
V3885 Sgr |oscillations are sometimes observed with
V3885 Sgr |P1 = 29.0s, P2 = 30.15s and with amplitudes of 0.00028m.
V3885 Sgr |In the spectrum there are extremely broad absorption
V3885 Sgr |lines of HI and HeI. The Balmer lines have emission
V3885 Sgr |components. X-ray source.
V3886 Sgr |Type EB?
V3893 Sgr |Connected with a ring nebula.
V3894 Sgr |Min II 6.37. P var?
V3899 Sgr |In the region of the open cluster and the diffuse nebula
V3899 Sgr |NGC 6514 (M20).
V3900 Sgr |V7 (NGC 6522). Not a member of this globular cluster.
V3903 Sgr |The member of the open cluster Collinder 367.
V3903 Sgr |In the nebula Simeis 188.
V3907 Sgr |The epoch of Min brightness is given.
V3929 Sgr |P.K.5 -5deg 2.
V3961 Sgr |SB1 (Porb = 690d [09915]).
V4024 Sgr |SB.
V4032 Sgr |Not far from V1309 Sgr.
V4034 Sgr |Flat Min. Close companion?
V4046 Sgr |Flares (11.1m - 12.4m U).
V4048 Sgr |Min II 12.6; DII = 0.15P.
V4051 Sgr |In the region of the globular cluster NGC 6638.
V4051 Sgr |Not a member of the cluster.
V4052 Sgr |In the region of the globular cluster NGC 6638.
V4052 Sgr |Not a member of the cluster.
V4054 Sgr |In the region of the globular cluster NGC 6638.
V4054 Sgr |Not a member of the cluster.
V4055 Sgr |In the region of the globular cluster NGC 6638.
V4055 Sgr |Not a member of the cluster.
V4058 Sgr |d = 0.02P
V4060 Sgr |P var. Max = 2437846 + 283d*E (JD2436030 - 38970);
V4060 Sgr |since JD2438970 - see Table.
V4066 Sgr |d ~0.07P.
V4067 Sgr |V32 (NGC 6656 = M22).
V4067 Sgr |Not a member of the globular cluster.
V4068 Sgr |V17 (NGC 6656 = M22).
V4068 Sgr |Not a member of the globular cluster.
V4069 Sgr |V33 (NGC 6656 = M22).
V4069 Sgr |Not a member of the globular cluster.
V4390 Sgr |SB2 and speckle binary.
V4417 Sgr |The variability may be due to the fainter (B) component.
V4429 Sgr |A giant, according to HIPPARCOS data, despite the published
V4429 Sgr |luminosity class (V).
V4955 Sgr |Close to the N of V4521 Sgr, the periods differ considerably.
V5099 Sgr |SU UMa-type cv.
V5112 Sgr |A symmetrical minimum lasted for several months, with variations also outside it.
eta   Sgr |VB A (B 8.0m, 3.5",105deg); mu alpha = -0.0107s,
eta   Sgr |mu delta = -0.166".
mu    Sgr |VB A (B 10.48m, 16.9", 285deg; C 13.0m, 25.2", 119deg;
mu    Sgr |D 9.69m, 48.5", 312deg; E 9.25m, 50.0", 115deg). SB2
mu    Sgr |(e = 0.4). The variability type is EA/GS + ACYG.
mu    Sgr |According to [09922] there are also quasiperiodical light
mu    Sgr |variations with the amplitudes 0.08m - 0.15m and cycles
mu    Sgr |from 16d to 40d.
ups   Sgr |Min II 4.59.
R     Sco |V7 (NGC 6093 = M80). Probable field star.
R     Sco |P var. Max = 2400518 + 220.2d*E (JD2400500 - 04000)
R     Sco |[00960]; Max = 2404493 + 225.86d*E (JD2404000 - 08600);
R     Sco |Max = 2409003 + 222.29d*E (JD2408600 - 33300); since
R     Sco |JD2433300 - see Table.
S     Sco |V6 (NGC 6093 = M80). Cluster non-member.
S     Sco |P var. Max = 2400986 + 177.00d*E (JD2400900 - 17500);
S     Sco |since JD2417500 - see Table.
T     Sco |4.0" N, 2.7" E from the center of the globular cluster
T     Sco |NGC 6093 = M80.
U     Sco |Previous outbursts:
U     Sco |2401646: (1863), 2417343 (1906), 2428342 (1936).
Y     Sco |Since 1972 varies its brightness in the range 12.3m-15.0m
Y     Sco |irregularly, maxima are unpredictable [08080].
Z     Sco |P var. Max = 2425546 + 357.17d*E (JD2412500 -
Z     Sco |25600); since JD2430000 - see Table.
RR    Sco |SiO maser. P var. Max = 2416944 + 284.31d*E
RR    Sco |(JD2411000 - 18000); Max = 2422828 + 278.09d*E
RR    Sco |(JD2422800 - 40000); since JD2440000 - see Table.
RU    Sco |P var. During JD2425000 - 40000 - see Table.
RV    Sco |VB A (B 13.0m, 5.9", 325deg).
RW    Sco |OH, H2O, SiO maser.
RY    Sco |P var, nonlinear term: +4.10d*10**(-6)*E**2. [A/H] = 0.2.
RY    Sco |VB A (B 10.70m, F8:, 13.8", 220.5deg, 1965;
RY    Sco |C 11.5m, 2.0", 102deg, 1964; D 11.43m, 24", 80deg).
RY    Sco |Combined brightness of AC is given.
RZ    Sco |P var. Max = 2413994 + 161.20d*E (JD2413600 - 22700);
RZ    Sco |Max = 2422858 + 155.79d*E (JD2422700 - 28000);
RZ    Sco |Max = 2428156  +  160.29d*E (JD2428000 - 35000); since
RZ    Sco |JD2437500 - see Table.
SV    Sco |P var. Max = 2418886 + 258.5d:*E (JD2411600 - 19000);
SV    Sco |Max = 2424233 + 252.43d*E (JD2420500 - 28600);
SV    Sco |Max = 2429055 + 255.9d:*E (JD2428600 - 35000);
SV    Sco |since JD2437000 - see Table.
SY    Sco |In the region of the open cluster NGC 6475 = M7.
TX    Sco |In the region of the open cluster NGC 6475 = M7.
TX    Sco |Probable cluster member.
XX    Sco |The elements Max = 2413786 + 152d*E
XX    Sco |[00031] do not represent the observations from [09447].
AC    Sco |According to [00266], CST:, 12.2m - 12.6m pg.
AH    Sco |OH, H2O, SiO maser.
AI    Sco |P2 = 966.6d.
AL    Sco |Min II 11.3.
AN    Sco |EA type is possible.
AP    Sco |The chart in [09447] is wrong.
AR    Sco |According to [07104], T Tau type spectrum.
AU    Sco |VB A (B = V725 Sco, 0.4', 0deg).
AV    Sco |The chart and data in [09447] correspond to another star.
BI    Sco |VB B (A = GW Sco; B 6", 150deg).
BM    Sco |In the region of the open cluster NGC 6405 = M6.
BN    Sco |In the region of the open cluster NGC 6475 = M7.
BN    Sco |Resembles R Cen.
BS    Sco |d <= 0.03P. According to [00021], SP F8.
BT    Sco |P var. There is periodic term in the elements given in the
BT    Sco |Table: +0.05d*sin(176deg + 0.0857deg*E). Blazhko effect?
BV    Sco |Doubtful identification in [09447].
CF    Sco |Min II 13.8.
CK    Sco |VB A (B 15m, 14").
CL    Sco |The brightness in optical and UV range is modulated
CL    Sco |according to the elements: Min (pg) = 2427020 + 624.7d*E.
CL    Sco |Outbursts 1892, 1899, 1907, 1926.
CP    Sco |N /= 4.
CQ    Sco |[A/H] = -1.4.
DX    Sco |VB A (B p).
EZ    Sco |VB A (B 15.6m nf).
FQ    Sco |VB A (B 16m vis).
FU    Sco |VB A (B np). Min II 12.7, Min II - MiN I = 0.493P.
FV    Sco |d = 0.015P. Depth of Min II 0.1m pg.
FY    Sco |VB A (B 15m, 15", 35deg).
GG    Sco |VB A (B 15m, 8", 45deg).
GM    Sco |The nothern one of the two stars noted on the chart for
GM    Sco |SVS 1677.
GW    Sco |VB A (B = BI Sco, 6", 150deg).
IU    Sco |VB A (B 16.4m nf).
IU    Sco |Max = 2413280 + 69.05d*E (1893 - 1906);
IU    Sco |during 1910 - 1928 - see Table.
KO    Sco |Rapid variations: A = 1.0m. Slow changes:
KO    Sco |A = 0.5m, P = 2000d +-.
KQ    Sco |[A/H] = +0.3. P var?
LO    Sco |P var? Before JD2419150 Max = 2411500 + 450d*E;
LO    Sco |since JD2423900 - see Table.
LO    Sco |The spectrum is later than M5.
LR    Sco |The spectrum resembles RCrB in Max light [08090].
LR    Sco |IR excess. RCB type minima were not observed.
OO    Sco |In the region of the open cluster TR 29.
OQ    Sco |The chart in [06286] is wrong.
QZ    Sco |P var. Before JD2420400 Max = 2412640 + 158d*E;
QZ    Sco |since JD2423900 - see Table.
V0347 Sco |P var. Before JD2418700 Max = 2411500 + 198d*E;
V0347 Sco |since JD2423900 - see Table.
V0381 Sco |d = 0.046P.
V0382 Sco |In the region of the open cluster NGC 6475 = M7.
V0385 Sco |In the region of the open cluster CR 338.
V0387 Sco |Min II 12.2.
V0390 Sco |P var. Before JD2422500 Max = 2420330 + 466d*E;
V0390 Sco |since JD2423900 - see Table.
V0393 Sco |Min II 8.3.
V0400 Sco |Min II 15.0.
V0402 Sco |In the region of the open cluster NGC 6475 = M7.
V0403 Sco |d ~0.02P. The depth of Min II 0.05m.
V0407 Sco |In the region of the open cluster NGC 6475 = M7.
V0411 Sco |Min II 14.0.
V0412 Sco |Min II 14.8. In the region of the open cluster
V0412 Sco |NGC 6475 = M7.
V0420 Sco |In the region of the open cluster NGC 6475 = M7.
V0421 Sco |P var. Before JD2418000 Max = 2413830 + 293d*E;
V0421 Sco |since JD2423900 - see Table.
V0423 Sco |Min II 14.2. In the region of the open cluster
V0423 Sco |NGC 6475 = M7.
V0425 Sco |In the region of the open cluster NGC 6475 = M7.
V0426 Sco |In the region of the open cluster NGC 6475 = M7.
V0429 Sco |In the region of the open cluster NGC 6475 = M7.
V0430 Sco |In the region of the open cluster Tr 30.
V0432 Sco |In the region of the open cluster Tr 30.
V0437 Sco |d = 0.02P. Min II 13.9.
V0439 Sco |P var. Before JD2418200 Max = 2413350 + 166.5d*E;
V0439 Sco |since JD2419900 - see Table.
V0440 Sco |In the region of the open cluster Tr 30.
V0446 Sco |P var? before JD2435000 Max = 2434980.1 +
V0446 Sco |28.6195d. [A/H] = -1.0.
V0450 Sco |A = 0.9m pg.
V0453 Sco |VB A (B 13.51m, F7V, 13.5", 168deg). Min II 6.70.
V0453 Sco |The light curve shape var?
V0455 Sco |P.K.351deg  + 3deg1. Planetary nebula nature is doubtful.
V0455 Sco |Nova-like outbursts separated by several years.
V0457 Sco |Min II 11.3.
V0460 Sco |d = 0.02P.
V0464 Sco |d = 0.03P.
V0466 Sco |Min II 13.7.
V0467 Sco |P var. P = 2.41354d (1889 - 1903); since 1903 - see Table.
V0470 Sco |[A/H] = 0.1.
V0471 Sco |Min II 15.2, dII = 0.08P(!).
V0472 Sco |d = 0.02P.
V0474 Sco |Min II 10.6.
V0483 Sco |CI = +3.5m.
V0485 Sco |Short term variations are superimposed.
V0486 Sco |D >= 4d? P = 1d is possible. In the region of
V0486 Sco |the open cluster NGC 6383.
V0487 Sco |[Fe/H] = -1.67, Delta(S) = 9.0.
V0490 Sco |Min II 12.5.
V0491 Sco |Min II 13.2.
V0494 Sco |A var (1.27m - 1.66m B). P var? Delta(S) = 2.
V0494 Sco |VB A (B 12.72m y, 23").
V0495 Sco |Short term variation are superimposed.
V0495 Sco |(Delta(m)short = 0.5m +-).
V0496 Sco |In the region of the open cluster NGC 6414.
V0496 Sco |d = 0.03P.
V0497 Sco |Min II 13.6.
V0499 Sco |AII = 0.47m V. Min I - Min II = 0.504P.
V0502 Sco |In the region of the open cluster C 1712 - 407.
V0507 Sco |The epoch of Max from [00300] contradicts the elements.
V0540 Sco |VB A (B 15.2m sp).
V0547 Sco |VB B (A 14.2m sf).
V0549 Sco |[A/H] = -1.1.
V0555 Sco |[A/H] = -0.3.
V0562 Sco |Min II 12.1.
V0566 Sco |d = 0.01P:.
V0567 Sco |VB A (B 13.01m, 10"sp, CD 30"nf). P var.
V0568 Sco |d = 0.04P.
V0569 Sco |Min II 11.4.
V0570 Sco |P var? Unusually broad Max.
V0573 Sco |d = 0.06P. In the region of the open cluster Tr 24.
V0574 Sco |In the region of the open cluster Tr 24.
V0575 Sco |Min II 12.4.
V0579 Sco |In the region of the open cluster Tr 24.
V0581 Sco |Min II 11.9.
V0584 Sco |Min II 13.1.
V0585 Sco |d = 0.03P:.
V0586 Sco |d = 0.04P. In the region of the open cluster Tr 24.
V0588 Sco |d = 0.02P. In the region of the open cluster Tr 24.
V0589 Sco |d = 0.05P. In the region of the open cluster Tr 24.
V0590 Sco |In the region of the open cluster NGC 6231.
V0592 Sco |Min II 13.3.
V0593 Sco |d = 0.05P:.
V0594 Sco |d = 0.01P.
V0603 Sco |d = 0.04P.
V0606 Sco |d = 0.07P.
V0607 Sco |Min II 10.3.
V0609 Sco |Min II 13.7.
V0611 Sco |d = 0.04P. Min II 13.7.
V0612 Sco |d = 0.05P.
V0613 Sco |d = 0.04P.
V0616 Sco |Min II 12.4.
V0619 Sco |Min II 12.1.
V0620 Sco |d = 0.02P.
V0621 Sco |d = 0.04P.
V0622 Sco |Min II 14.2.
V0623 Sco |Long intervals in Max without changes, sometimes becomes
V0623 Sco |faint.
V0625 Sco |VB A (B 13.2m sf). Min II 13.5.
V0627 Sco |Min II 14.1.
V0628 Sco |Min II 12.4.
V0629 Sco |Apsidal motion.
V0631 Sco |Min II 13.2.
V0632 Sco |d = 0.06P.
V0633 Sco |Min II 12.2.
V0634 Sco |Min II 12.2.
V0636 Sco |SB1 (Porb = 1318d).
V0638 Sco |d = 0.07P.
V0640 Sco |Min II 13.5.
V0656 Sco |The chart in [06286] is wrong.
V0660 Sco |VB A (B 16.0m s).
V0672 Sco |P = 180d is possible.
V0674 Sco |VB A (B 15.0m s).
V0677 Sco |The chart in [06286] is wrong.
V0679 Sco |P = 364d is possible.
V0690 Sco |VB A (B 14.40m y, 6", 0deg). The range of the combined
V0690 Sco |light is given. Delta(S) = 4.
V0698 Sco |D <= 0.20d, d = 0.043d.
V0700 Sco |Min II 10.3.
V0701 Sco |Min II 9.05. P var. Min I = 2439329.6657 + 0.76187133d*E
V0701 Sco |(JD2428000 - 39400) [07177]; since JD2439400 - see Table.
V0701 Sco |Probable member of the open cluster NGC 6383.
V0702 Sco |Probable member of the open cluster NGC 6383.
V0703 Sco |P0 = 0.1499615d [03521]; P1 - see Table
V0703 Sco |(P var?). Also noted P = 0.04162025d [03521].
V0703 Sco |A var (0.23m - 0.46m). Beat phenomenon:
V0703 Sco |Max = 2436760.249 + 0.497306d*E [03521]. Delta(S) = 1.
V0703 Sco |In the region of the open cluster NGC 6405 = M6.
V0705 Sco |Min II 14.1:.
V0706 Sco |Moments of Max from [00046] contradict the tabulated
V0706 Sco |elements. According to [04678], A <= 0.05m V
V0706 Sco |during 6 nights.
V0708 Sco |In the region of the open cluster NGC 6475 = M7.
V0709 Sco |IN the region of the open cluster NGC 6475 = M7.
V0709 Sco |[A/H] = -0.6.
V0710 Sco |Min II 14.2.
V0711 Sco |In the region of the open cluster NGC 6475 = M7.
V0712 Sco |Min II 14.0.
V0714 Sco |d = 0.05P:. P may be twice longer.
V0717 Sco |[A/H] = 0.9.
V0718 Sco |D ~4d. Another Min 2429847 - 849 [00270].
V0720 Sco |In the region of the open cluster NGC 6475 = M7.
V0723 Sco |In the region of the open cluster NGC 6475 = M7. At the
V0723 Sco |edge of a dark cloud.
V0725 Sco |VB B (A = AU Sco, B 0.4', 0deg).
V0729 Sco |Possibly a Nova.
V0732 Sco |P may be twice longer.
V0733 Sco |Possibly a Nova.
V0734 Sco |Possibly a Nova.
V0735 Sco |The light curve shape var.
V0738 Sco |d = 0.04P:; Min II 13.4:. In the region of the open
V0738 Sco |cluster NGC 6475 = M7.
V0740 Sco |In the region of the open cluster NGC 6475 = M7.
V0741 Sco |There is a red variable close to the coordinates in the
V0741 Sco |discovery announcement [02448], but a different star is
V0741 Sco |marked in the chart in [02448].
V0749 Sco |P = 410d is possible.
V0756 Sco |Min II 10.7.
V0760 Sco |dI = 0.02P; Min II 7.4; DII = 0.2P:, dII = 0.03P.
V0761 Sco |IN type is not excluded.
V0764 Sco |Min II 9.0.
V0805 Sco |Possibly P is twice shorter.
V0818 Sco |Sco X-1. SB.
V0818 Sco |Var X-ray and multi-component radio source.
V0818 Sco |Lx/Lbol = 300 - 1000. The epoch of Min is
V0818 Sco |given for the periodic component of the light variation
V0818 Sco |(A ~0.25m). Flickering and flares up to 1m with
V0818 Sco |time scale from dozens of seconds to minutes. The
V0818 Sco |mean brightness level decreased in the middle of
V0818 Sco |1960-es by 0.3m-0.4m. The spectrum with blue continuum
V0818 Sco |and H, HeI, HeII, CIII, NIII emissions.
V0819 Sco |Min II 13.2.
V0821 Sco |Min II 14.5.
V0822 Sco |VB? Combined brightness.
V0827 Sco |Min II 14.1.
V0833 Sco |Min II 11.2.
V0837 Sco |d ~0.03P:; Min II 14.3.
V0838 Sco |Min II 13.4.
V0842 Sco |Min II 12.3.
V0843 Sco |Min II 10.5.
V0848 Sco |Min II 13.1. RRC type with twice shorter period is
V0848 Sco |possible.
V0849 Sco |Min II 14.1.
V0853 Sco |d = 0.05P; Min II 14.1.
V0856 Sco |VB C (A = BS 6000, 6.65m, AO-3III; B 12.55m, 16",
V0856 Sco |298deg; C 44", 185deg; D 11.7m, CD 1.3", 105deg, 1945).
V0857 Sco |Erroneously labelled "10" (instead of "11") in the chart.
V0858 Sco |Erroneously labelled "11" (instead of "10") in the chart.
V0861 Sco |SB1. Min II 6.28. Depths of minima var. In the region of
V0861 Sco |the open cluster NGC 6231, Cr 316, Tr 24.
V0862 Sco |Usually 6.67m - 6.76m. A flare of 40m duration on July 3,
V0862 Sco |1965. In the region of the open cluster NGC 6405 = M6.
V0866 Sco |VB (Delta(m) ~0.5m, ~1", 200deg). m (6370 A) =
V0866 Sco |11.14m - 12.37m. IR excess.
V0870 Sco |B-V =  +3.38m - +3.52m. In the region of the open cluster
V0870 Sco |NGC 6231.
V0877 Sco |Min II 13.1.
V0883 Sco |VB A (B 12.60m, 9", 130deg). P var?
V0883 Sco |Min = 2438228.315 + 1.294745d*E (JD2438200 - 40500)
V0883 Sco |[06871]; since JD2440500 - see Table. Deep Min II.
V0884 Sco |4U 1700-37. LX/Lbol = 0.00007.
V0884 Sco |Eclipsing X-ray source. Eclipse duration is variable
V0884 Sco |in the ranges 0.61d <= dx <= 1.10d. The epoch of the
V0884 Sco |middle of the X-ray eclipse coinciding with Min II is
V0884 Sco |given. X-ray flux var in the scale from seconds till
V0884 Sco |hours. Sometimes a periodic modulation with P ~97
V0884 Sco |Min is present, its amplitude in the optical band reaches
V0884 Sco |Delta(V) ~0.01m. Min II 6.57; Min I - Min II = 0.63P,
V0884 Sco |dI=0.2P. Surrounded by the ring nebula Sh 2. in the region
V0884 Sco |of the open cluster NGC 6281. Field star.
V0885 Sco |Noticeable Min II.
V0889 Sco |The northern component of a triple.
V0890 Sco |VB A (B 11.5m, 0.5' n).
V0894 Sco |A = 0.6m pg.
V0896 Sco |Co-ordinates or the chart may be erroneous.
V0900 Sco |In the region of the open cluster NGC 6231.
V0900 Sco |The light curve is a sinusoidal wave. Possibly
V0900 Sco |P = 6.20d; 6.85d.
V0903 Sco |N96 [02448]. Erroneously identified with V479 Sco.
V0906 Sco |In the region of the open cluster NGC 6475 = M7. Probable
V0906 Sco |cluster member. VB (delta(mV) = 0.8m, 0.1", 111deg, 1957).
V0906 Sco |The range of the combined light variation is given.
V0906 Sco |Min II 6.21.
V0907 Sco |In the region of the open cluster NGC 6475 = M7.
V0907 Sco |Min II 9.2.
V0911 Sco |Alternative P = 4.2d.
V0913 Sco |Alternative P = 0.976d. IR excess.
V0914 Sco |VB (delta(mV) = 2m, 3", 200deg). Sine wave with P = 2.69d,
V0914 Sco |Delta(B) = 0.15m (B = 12.91m) [09753].
V0915 Sco |VB A (B 10.43m, WN6, 14", 330deg; C 11.40m, 20", 202deg;
V0915 Sco |D 13.96m, 22", 80deg, 1973). The brightness decreased from
V0915 Sco |6.32m to 6.50m during JD2443680 - 44115.
V0917 Sco |VB A (B 17m: sp). The outburst: rise 1930-1936,
V0917 Sco |Max 1936-1938, decline 1938-1952.
V0919 Sco |In the region of the open cluster NGC 6231.
V0920 Sco |In the region of the open cluster NGC 6231. Multiple
V0920 Sco |periodicity: P1 - see Table, semiamplitude A1 = 0.0051m;
V0920 Sco |P2 = 0.10765d. A2 = 0.0046m; P3 = 0.10388d, A3 = 0.00485m;
V0920 Sco |P4 = 0.12137d, A4 = 0.0036m; P5 = 0.6929d?, A5 = 0.0028m.
V0921 Sco |The star illuminates a nebula.
V0922 Sco |Multiple periodicity, superposition of frequencies with
V0922 Sco |amplitudes 0.0010m - 0.0352m.
V0923 Sco |D = 0.32d:. The elements need confirmation. In the region
V0923 Sco |of the open cluster NGC 6281.
V0924 Sco |B-V var: +1.90, +2.50,
V0924 Sco |Light fluctuations by 0.1m - 0.2m (u, b) in several
V0924 Sco |minutes.
V0925 Sco |VB A (B ~10", faint, blue). Probable member of the open
V0925 Sco |cluster TR 27. In Vr possible values of P: 105.3d, 73.0d,
V0925 Sco |188.7d, 312.5d [09950].
V0926 Sco |3U 1735-44 = Sco XR-3. Bursts superimpose small light
V0926 Sco |variations with P = 0.18d which is apparently the
V0926 Sco |orbital period [04394].
V0927 Sco |The epoch of Min in U light is given. IR excess.
alf   Sco |ADS 10074 A(B 5.1m, B4Ve, A = 2.9", Porb = 878 yr.).
alf   Sco |Connected with a nebula.
zet 1 Sco |In the region of the open cluster NGC 6231.
kap   Sco |SB. P2 = 0.205430d. P1 var. Beat phenomenon:
kap   Sco |Pi = 7.3316d.
lam   Sco |SB1. Porb = 5.6d? Apuls = 0.02m. Long period light changes:
lam   Sco |Max = 2440376.15 + 10.1605d*E [09761]. One eclipse was
lam   Sco |found (JD2440690, A ~0.04m) [06388].
mu  1 Sco |Min II 3.12.
sig   Sco |VB AA (A 5.5m, 0.37", 96deg, 1981,
sig   Sco |orbital motion?; B 8.45m, B9.5V, 20.1", 273deg,
sig   Sco |1961); SB1, Porb = 33.06d. P0 var.
sig   Sco |Max Vr = 2420000.1465 + 0.24682815d*E (1918 - 1924)
sig   Sco |[09953]; Max = 2432306.918 + 0.246846d*E (JD2432000 - 37800)
sig   Sco |[09764]; since JD2437800 - see Table.
sig   Sco |A0 = 0.036m y. P1 = 0.2396674d, A1 = 0.013m y [09762].
sig   Sco |Pbeat = 8.256d = Porb/4 [09957].
sig   Sco |Connected with a nebula.
R     Scl |VB A (B 19.9m, 10", 234deg). CO emission.
S     Scl |P var. Max = 412774 + 367.9d*E (JD2405400 - 20500);
S     Scl |Max = 2423035 + 360.6d*E (JD2421250 - 27740);
S     Scl |Max = 2427738 + 370.4d*E (JD2427700 - 34000) [00960];
S     Scl |Since JD2434000 - see Table. H2O emission.
T     Scl |P var. Max = 2417400 + 202.26d*E (JD2411300 - 19000);
T     Scl |Max = 2420390 + 197.85d*E (JD2419000 - 23600);
T     Scl |since JD2423600 - see Table.
V     Scl |P var. Max = 2414006 + 294.8d*E (JD2411600 - 18200);
V     Scl |Max = 2422866 + 297.2d*E (JD2420400 - 35100);
V     Scl |since JD2435100 - see Table.
X     Scl |P var. Max = 2413796 + 258.7d*E (JD2413500 - 22800);
X     Scl |since JD2422800 - see Table.
Y     Scl |The cycles 100d: and 300d: are sometimes observed.
RT    Scl |Min II 10.47. [Fe/H] = -0.75. P var. There is
RT    Scl |a nonlinear term in the elements given in the Table:
RT    Scl |-9.04d*10**(-11)*E**2.
RU    Scl |(k - b)2 = 0.09. A var [03429]. P var. Max = 2425094.4175 +
RU    Scl |0.4933257d*E (JD2416750 - 25100) [00183]; Max =
RU    Scl |2427403.177 + 0.4933239d*E (JD2425100 - 30650)
RU    Scl |[01381]; since JD2430650 - see Table.
RW    Scl |P var?
SV    Scl |[Fe/H] = -1.82. P var? Max = 2439468.364 +
SV    Scl |0.3773636d*E (JD2427300 - 39500) [05233];
SV    Scl |since JD2439850 - see Table.
SY    Scl |H2O maser. P var? Max = 2426160 + 411d*E [00193]; since
SY    Scl |JD2440400 - see Table.
SZ    Scl |Min II 13.68.
UY    Scl |Near the galaxy NGC 55.
UZ    Scl |VB A (B 15.81m, 23", 135deg); (k - b)2 = 0.14. The
UZ    Scl |shape of the light curve varies.
VV    Scl |Min II 8.50. ACV? [08083].
VY    Scl |Porb = 0.1662d? [09932]. High and low states of the
VY    Scl |system are observed.
VZ    Scl |High and low states of the system are observed [09933].
WZ    Scl |There are two oscillations with the periods P1 and
WZ    Scl |P2: P1 = 0.06576d, P2 = 0.095944d, P1/P2 = 0.6854.
XX    Scl |There are two oscillations with the periods P1 and
XX    Scl |P2: P1 = 0.048898d, P2 = 0.051350d, P1/P2 = 0.95225.
AI    Scl |There are two oscillations with the periods P1 and
AI    Scl |P2: P1 = 0.044d, P2 = 0.0931d, P1/P2 = 0.47.
AL    Scl |Min II 6.20; Min II - Min I = 0.475P; DII = 0.08P.
AO    Scl |mu = 0.46", P = 187deg.
BC    Scl |May be eclipsing.
BI    Scl |Type E: is also possible.
R     Sct |[Fe/H] = -1. P var. Min I = 2377165 + 142.8d*E
R     Sct |(JD2377160 - 9820); Min I = 2384885 + 142.6d*E
R     Sct |(JD2384890 - 8170); Min I = 2394451 + 141.4d*E
R     Sct |(JD2394450 - 8500); Min I = 2398777 + 142.4d*E
R     Sct |(JD2398770 - 2404320); Min I = 2404627 + 137.4d*E
R     Sct |(JD2404600 - 6410); Min I = 2406561 + 142.7d*E
R     Sct |(JD2406560 - 9065); Min I = 2409742 + 143.6d*E
R     Sct |(JD2409730 - 12700); Min I = 2412755 + 141.5d*E
R     Sct |(JD2412750 - 16720); Min I = 2417161 + 139.5d*E
R     Sct |(JD2417150 - 20790); Min I = 2421083 + 143.4d*E
R     Sct |(JD2421050 - 25170) [09935]; Min I = 2429478 + 142.8d*E
R     Sct |(JD2429000 - 30650) [09938]; Min I = 2432078 + 140.05d*E
R     Sct |(JD2432000 - 42240) [07596]; Min I = 2442737 + 152.5d*E
R     Sct |(JD2442550 - 43050); Min I = 2443315 + 138.5d*E
R     Sct |(JD2443050 - 44150) [00001]; since JD2444150 - see Table.
R     Sct |Light curve drawings [09935,09936,9937].
R     Sct |Spectrum description [09939,09954].
S     Sct |VB A (B 11.9M V, 14.5", 238deg; C 12.5m V, 44", 105deg).
U     Sct |Min II 10.31.
W     Sct |Min II 10.1.
X     Sct |[A/H] = -0.1. In the region of the open cluster NGC 6639.
Y     Sct |In the region of the open cluster NGC 6664.
Z     Sct |[A/H] = 0.3.
RS    Sct |Min II 10.08.
RU    Sct |[A/H] = -0.7. P var. There is a nonlinear term in the
RU    Sct |elements given in the Table: +3.15d*10**(-6)*E**2.
RX    Sct |Connected with the bright hydrogen nebula YM 13.
RY    Sct |Min II 9.56. P var? Min I = 2427979.340 + 11.124939d*E
RY    Sct |(JD2414800 - 36100) [00007]; since JD2431200 - see Table.
RY    Sct |The shape of the light curve varies.
RZ    Sct |Min II 7.47. P var. There is nonlinear term in the
RZ    Sct |elements given in the Table: +0.78d*10**(-7)*E**2.
SU    Sct |P var. Max = 2424324.48 + 1.467713d*E (JD2420700 - 34310);
SU    Sct |Max = 2439678.428 + 1.468753d*E (JD2437100 - 41100) [07806];
SU    Sct |since JD2441100 - see Table.
TX    Sct |CWA? red.
TY    Sct |[A/H] = -0.3. In the region of the open cluster Tr 35.
UZ    Sct |[Fe/H] = 0.35. P var. Max = 2435629.5 + 14.7468d*E
UZ    Sct |(JD2423900 - 35700) [02309]; since JD2436000 - see Table.
VV    Sct |SF component of a pair.
VW    Sct |P var. Max = 2415887 + 234d*E (JD2411900 - 22210);
VW    Sct |Max = 2423588 + 235d*E (JD2422880 - 27600);
VW    Sct |Max = 2429468 + 235.1d*E (JD2428750 - 34200);
VW    Sct |since JD2434600 - see Table.
VX    Sct |d = 0.064P.
VZ    Sct |Min II 12.0.
WY    Sct |P var.
XY    Sct |Min II 14.5.
AC    Sct |d = 0.024P; Min II 10.2.
AE    Sct |d = 0.04P.
AI    Sct |In the region of the open cluster NGC 6705.
AN    Sct |P var?
AP    Sct |V2 (NGC 6712).
AU    Sct |d ~0.03P.
BC    Sct |Following component of a close double system. The
BC    Sct |companion - NSV 11551.
BH    Sct |Min II 14.9.
BI    Sct |VB A (B 16.3m:, 3", 280deg; C 16.7m:, 12", 190deg;
BI    Sct |D 16.8m:, 18", 45deg; E 17.0m:, 6", 350deg).
BK    Sct |Close companion 16.5m sf.
BN    Sct |d = 0.02P.
BP    Sct |S 5.5/5.5.
BS    Sct |Min II 11.07. In the region of the open cluster M11
BS    Sct |(NGC 6705).
BU    Sct |A var. P var. Max = 2425804.625 + 0.42022d*E [01401];
BU    Sct |Max = 2427928.041 + 0.4202188d*E (JD2427900 - 9440)
BU    Sct |[01404]; Max = 2432770.464 + 0.4201944d*E
BU    Sct |(JD2432740 - 38290); Max = 2438589.357 + 0.4202171d*E
BU    Sct |(JD2438580 - 40510) [07806]; since JD2440770 - see Table.
BX    Sct |[A/H] = -0.9.
CD    Sct |Min II 13.7.
CF    Sct |d = 0.035P.
CH    Sct |V7 (NGC 6712). The member of this globular cluster.
CK    Sct |[Fe/H] = 0.23.
CL    Sct |May be the period should be doubled?
CM    Sct |[A/H] = 0.1.
CN    Sct |[A/H] = -1.5.
CO    Sct |P var? Resembles RV Tau type variables: if the period is
CO    Sct |doubled, the neight of max I and the depth of Min II vary.
CR    Sct |Min II 12.1; DII = 0.071P; Min II - Min I = 0.53P.
CT    Sct |Min II 11.1.
CW    Sct |Min II 10.1.
CZ    Sct |The epoch of Min brightness is given.
DD    Sct |One of the components probably varies.
DE    Sct |Min II 16.3.
DG    Sct |d = 0.03P:.
DL    Sct |Min II 15.9.
DT    Sct |Min II 16.5.
DV    Sct |Min II 17.8.
DW    Sct |Min II 16.4.
EE    Sct |Min II 15.3.
EH    Sct |Min II 15.0.
EK    Sct |Min II 16.0.
EL    Sct |The shape of the light curve varies?
EN    Sct |Min II 17.2. The different elements are also possible:
EN    Sct |Min I = 2428008.85 + 1.06446d*E.
EP    Sct |d = 0.04P:; Min II 15.6.
EQ    Sct |In the region of the open cluster NGC 6631. Min II 12.6:.
ER    Sct |Min II 9.3; Min II - Min I = 0.506P; DII = 0.14P.
EU    Sct |VB A (B 17.5m, 6", 45deg).
EV    Sct |[A/H] = -0.4. The member of the open cluster NGC 6664.
EW    Sct |P0 = 5.8195d (A/2 = 0.27m), P1 = 4.0646d (A/2 = 0.22m);
EW    Sct |P1/P0 = 0.6984.
EX    Sct |d = 0.025P:.
EY    Sct |Min II 12.4. In the region of the open cluster NGC 6683.
EZ    Sct |Min II 12.5.
FF    Sct |Min II 14.2.
FG    Sct |Min II 14.70. P var? Min I = 2429017.557 + 0.2705728d*E
FG    Sct |(JD2427975 - 29520) [01397]; since JD2444700 - see Table.
FH    Sct |In the region of the open cluster NGC 6694.
FK    Sct |Min II 14.4:.
FL    Sct |Min II 13.8.
FM    Sct |Min II 12.9.
FN    Sct |In the open cluster NGC 6704.
FO    Sct |D = 0.22d.
FR    Sct |Spectrum description [01410].
GI    Sct |Min II 14.5.
GM    Sct |Min II 13.8:.
HI    Sct |D = 0.29d.
HL    Sct |Min II 13.4.
IS    Sct |P < 200d.
IT    Sct |In the region of the open cluster NGC 6705.
LL    Sct |sf component of a close pair.
LR    Sct |In the region of the globular cluster NGC 6712.
LU    Sct |P2 = 30d.
LZ    Sct |In the region of the globular cluster NGC 6712.
MM    Sct |Min II 15.8.
MP    Sct |V1 (NGC 6712). The member of this globular cluster.
MP    Sct |[Fe/H] = -0.69.
MR    Sct |V8 (NGC 6712). P var. Max = 2430885 + 117d*E
MR    Sct |(JD2427900 - 32400) [04231]; since JD2434900 - see Table.
NU    Sct |VB A (B 16.6m, 12", 180deg).
NV    Sct |P = 200d?
OU    Sct |P var. Max = 2427620 + 152d*E (JD2426200 - 32800);
OU    Sct |since JD2433100 - see Table.
PT    Sct |There is a close companion, 16.4m.
PW    Sct |The range of the combined light of the variable and
PW    Sct |a close companion, which follows, is given in the Table.
QU    Sct |The variable is also eclipsing one with P = 0.2d and
QU    Sct |A = 0.7m.
V0337 Sct |A close companion (16.2m, <7", 90deg).
V0340 Sct |Min II 15.6.
V0356 Sct |Min II 12.3; DII = 0.10P.
V0360 Sct |A close fn companion, 16.4m.
V0362 Sct |P = 170d?
V0367 Sct |In the open cluster NGC 6649. The light elements
V0367 Sct |with fundamental mode period P0 (A0 = 0.54m B) are
V0367 Sct |given in the Table. For the first-overtone period
V0367 Sct |P1 (A1 = 0.41m B) Max = 2437435.12 + 4.38466d*E;
V0367 Sct |P1/P0 = 0.696744. M - m var (0.15 <= M - m <= 0.45).
V0369 Sct |In the region of the open cluster NGC 6705 (M 11).
V0369 Sct |There is a superposition of the four light oscillations:
V0369 Sct |P1 = 0.240d (A1 = 0.044m), P2 = 0.220d (A2 = 0.020m),
V0369 Sct |P3 = 0.182d (A3 = 0.068m), P4 = 0.114d (A4 = 0.028m)
V0369 Sct |[09745].
V0370 Sct |d = 0.016P.
V0372 Sct |d = 0.012P.
V0414 Sct |Blue companion?
del   Sct |VB A (B 10m, 53", 130deg); (k - b)2 = 0.37.
del   Sct |The basic light variation P0 (A0 = 0.125m) given in the
del   Sct |Table is superposed by the secondary one with
del   Sct |P1 = 0.1867756 (A1 = 0.034) [09975].
R     Ser |P var. Max = 2372429 + 356.93d*E (JD2372400 - 88900)
R     Ser |[00960]; Max = 2397809 + 353.00d*E
R     Ser |(JD2394000 - 2403000); Max = 2403104 + 357.25d*E
R     Ser |(JD2403000 - 24000); Max = 2432387 + 356.10D*E
R     Ser |(JD2424000-39200); since JD2441000 - see Table.
R     Ser |Maser (SiO, H2O).
S     Ser |P var. Max = 2394360 + 361.01d*E (JD2394000 - 2407000);
S     Ser |Max = 2407024 + 372.70d*E (JD2407000 - 17000) [00960];
S     Ser |Max = 2425875 + 366.59d*E (JD2417000 - 36000); since
S     Ser |JD2437600 - see Table. Maser (OH, SiO, H2O).
T     Ser |In the region of the open cluster NGC 6633.
T     Ser |P var. Max = 2400907 + 342.05d*E (JD2400500 - 15000);
T     Ser |Max = 2417912 + 345.73d*E (JD2417900 - 26000);
T     Ser |Max = 2428524 + 332.21d*E (JD2426000 - 32500);
T     Ser |Max = 2438382 + 345.71d*E (JD2432500 - 39500); since
T     Ser |JD2439500 - see Table. 0.8' from BN Ser.
U     Ser |P var. Max = 2421158 + 237.70d*E (JD2414000 - 22000);
U     Ser |Max = 2422347 + 236.78d*E (JD2422000 - 26600);
U     Ser |Max = 2426609 + 239.21d*E (JD2426600 - 32500);
U     Ser |since JD2432500 - see Table.
V     Ser |Min II 9.85.
W     Ser |P var, nonlinear terms:
W     Ser |+(3.140d*10**(-6))*E**2 + (1.432d*10**(-9))*E**3.
W     Ser |The light curve shape var. Wavelike variations in Max
W     Ser |light. Changes of emission lines with the orbital phase.
W     Ser |Active mass exchange, evidence for a common envelope.
X     Ser |After 1932 variations 14.3m - 18.3m were noted; according
X     Ser |to [01417], P = 275d. Observations in 1961 - 1964 did not
X     Ser |confirm P = 275d, fluctuations of light with a period of
X     Ser |several minutes were suspected [03625]. The spectral data
X     Ser |are for 1981.
Y     Ser |Epoch of min is given. According to [08643], variations
Y     Ser |with P ~400d are superimposed by P ~40d.
Z     Ser |The elements are valid during JD2422000 - 31000.
RS    Ser |Min II 11.4.
RT    Ser |Max (1920 - 1923). In the spectrum (1977 - 1979) there are
RT    Ser |emissions Halpha - Hdelta, HeI, HeII, [OI] etc.
RT    Ser |Absorptions TiO.
RV    Ser |Maser (H2O).
VY    Ser |[Fe/H] = -1.77, Delta(S) = 9.
WW    Ser |Maser (H2O).
WX    Ser |Maser (OH, SiO, H2O). P var?
AA    Ser |[A/H] = 0.2.
AG    Ser |P var? since JD2435000 - see Table.
AK    Ser |P var? before JD2442300 Min = 2431313.266 + 1.9225667d*E
AK    Ser |[00318]; since JD2442300 - see Table.
AN    Ser |P var? Max = 2429156.260 + 0.5220703d*E
AN    Ser |(JD2427000 - 38000) [00001]; since JD2438000 - see Table.
AN    Ser |According to [02740], Blazhko effect with Pi = 21.94d;
AN    Ser |the presence of the Blazhko effect is denied in [07258].
AN    Ser |Delta(S) = 0.
AO    Ser |Min II 10.8.
AP    Ser |VB A (B 14.29m, 8" sp). [Fe/H] = -1.37.
AQ    Ser |Min II 11.1.
AR    Ser |P var. Before JD2425000 Max = 2415617.698 + 0.5752221d*E;
AR    Ser |Max = 2425313.530 + 0.57508945d*E
AR    Ser |(JD2425000 - 28500); Max = 2428848.662 + 0.575214d*E
AR    Ser |(JD2428500 - 31000) [08081]; Max =
AR    Ser |2431436.424 + 0.5751134d*E (JD2431000 - 34200);
AR    Ser |Max = 2436013.279 + 0.5752169d*E (JD2435900 - 37200);
AR    Ser |Max = 2438138.467 + 0.5750651d*E (JD2437200 - 38700)
AR    Ser |[00001]. Elements working on average since JD2438700 - see
AR    Ser |Table. Complex Blazhko effect. Pi = 108.4d [08082].
AR    Ser |A var (0.23m - 0.87m V). Pi var (80d - 120d) [07032].
AR    Ser |Delta(S) = 4.6.
AS    Ser |Min II 11.5. The epoch of Min I 2442937.428
AS    Ser |(BBSAG) is not in agreement with the elements.
AT    Ser |P var. Max = 2415353.783 + 0.74655695d*E
AT    Ser |(JD2415000 - 27000); Max = 2428337.260 + 0.7465670d*E
AT    Ser |(JD2428000 - 39500); since JD2441500 - see Table.
AT    Ser |Delta(S) = 9.
AU    Ser |Min II 11.61.
AU    Ser |The light curve shape var.
AV    Ser |Delta(S) = 6.
AW    Ser |Delta(S) = 5.0.
BF    Ser |[A/H] = -2.5. Delta(S) = 6.
BH    Ser |P var. Max = 2427956.674 + 0.434545d*E (JD2425000 -
BH    Ser |30700) [01039]; since JD2437650 - see Table.
BI    Ser |Min I 2446264.414 [10200] contradicts the elements. P var?
BN    Ser |In the region of the open cluster NGC 6633. 0.8' from
BN    Ser |T Ser.
BO    Ser |P var? Max = 2425681 + 201d (JD2425600 - 30100)  0447];
BO    Ser |the Table gives mean elements (JD2425600 - 35400).
BQ    Ser |P0 - see Table. P1 = 3.012d [08188]. In the region of the
BQ    Ser |open cluster IC 4756.
BR    Ser |In the region of the open cluster IC 4756.
BS    Ser |In the region of the open cluster IC 4756.
BT    Ser |In the region of the open cluster IC 4756.
BU    Ser |In the region of the open cluster IC 4756.
CC    Ser |Min II 11.63.
CN    Ser |[Fe/H] = -0.77. Delta(S) = 3.4.
CO    Ser |P var? The light curve shape var.
CO    Ser |[Fe/H] = -1.38. Delta(S) = 7.2.
CQ    Ser |Min II 12.0.
CR    Ser |[A/H] = -0.2.
CS    Ser |P var. Max = 2418137.875 + 0.5267904d*E
CS    Ser |(JD2416000 - 32500) [00001]; since JD2432500 - see Table.
CS    Ser |Delta(S) = (6). In the region of the HII complex S 54 and
CS    Ser |the open star cluster NGC 6604. Connected with a
CS    Ser |shell-structure nebula. Sometimes eclipses are observed
CS    Ser |during the configuration "WR in front of O" (see Table)
CS    Ser |and sometimes during the configuration "O in front of
CS    Ser |WR" which coincided with the deepest eclipse ever observed
CS    Ser |(with the depth 0.5m B, V). Sometimes the photometric
CS    Ser |eclipse at predicted moments does not occur, and only the
CS    Ser |atmospheric eclipse of the O star with the WR component is
CS    Ser |observed at lambda 4653 A (emission of CII - CIV, NIII),
CS    Ser |lambda < 2000 A. IR excess; possibly an IR eclipse in
CS    Ser |the configuration "O  in front of WR".
CX    Ser |The light curve (resembling the eclipsing light curve of
CX    Ser |U Gem) shows a hump of ~0.2m height before the minimum;
CX    Ser |fluctuations up to ~0.3m - 0.4m in Max.
DF    Ser |VB A (B 13.9m, 0.4', -115deg).
DG    Ser |Min II 16.5:. The alias period is possible (0.3360742d).
DH    Ser |Another possible P = 450d.
DK    Ser |Max 2433829 [10008] contradicts the elements.
DR    Ser |VB A (B 12.54m, 28", 0deg).
DT    Ser |VB A (B ~5"). The spectrum shows emissions of [OIII]
DT    Ser |lambda lambda 4959, 5007 A. Symbiotic? [08676].
DV    Ser |In a small star cluster.
DY    Ser |[Fe/H] = -1.58. Delta(S) = 8.4.
EE    Ser |In the region of the open cluster M 17 = NGC 6618.
EF    Ser |In the region of the open cluster M 17 = NGC 6618.
EG    Ser |VB A (ro > 10").
EL    Ser |N <= 7.
EN    Ser |[Fe/H] = -1.07. Delta(S) = 5.3.
EO    Ser |The light curve shows large scatter. RR(B) type is
EO    Ser |possible. Max = 2437433.653 + 0.6309d*E (JD2437433 - 514)
EO    Ser |[3625]. [Fe/H] = -1.63. Delta(S) = 8.8.
ER    Ser |In the region of the open cluster M 16 = NGC 6611.
ES    Ser |In the region of the open cluster M 16 = NGC 6611.
ET    Ser |In the region of the open cluster M 16 = NGC 6611.
EU    Ser |VB A (B 4" np). A member of the open cluster
EU    Ser |M 16 = NGC 6611. IR excess.
EV    Ser |In the region of the open cluster M 16 = NGC 6611.
EW    Ser |In the region of the open cluster M 16 = NGC 6611.
EX    Ser |In the region of the open cluster M 16 = NGC 6611.
FI    Ser |Hints of periodicity in U light.
FK    Ser |VB (Delta(m) ~0.5m, 1.3", 11.5deg, 1972).
FK    Ser |Flares were found in the satellite UV range [10013].
FK    Ser |Differences from typical by stars and probable "post-T Tau"
FK    Ser |nature are noted [07260,03866]. According to [06948],
FK    Ser |Min = 2441939.200 + 5.20d*E. Soft X-ray source.
FL    Ser |VB (Delta(m) = 1.9m, 0.46", 145deg, 1981).
FM    Ser |In the region of the open cluster M 16 = NGC 6611.
FM    Ser |VB (var sf?).
FN    Ser |In the region of the open cluster M 16 = NGC 6611.
FR    Ser |ADS 11477 A (B 12.5m, 10.5", 330deg, 1924; C 9.3m,
FR    Ser |30.5", 5deg, 1930). Possible values of P: 2.1308d, 2.1565d.
LN    Ser |m pg ~17.5m ~const; blue companion? [07264].
LS    Ser |The light curve shows large scatter, the elements need
LS    Ser |confirmation. Possible identification with an X-ray source
LS    Ser |2ASE 1822 + 0.
LV    Ser |The epoch of max in V light is given; in B and U varies
LV    Ser |in opposite phase.
LX    Ser |The depth of eclipses ~2.5m. Comparatively frequent
LX    Ser |outbursts [10023].
MM    Ser |Ser X-1 = 4 U 1 837 + 04. LX/Lopt >= 100.
MM    Ser |VB B (A 19.1m; B 2.2", 210deg).
MO    Ser |V1 (NGC 6535). Cluster non-member.
MP    Ser |V2 (NGC 6535). Cluster non-member.
OU    Ser |SB2.
PS    Ser |Both components are SB systems, Porb(A) = 15.888d,
PS    Ser |Porb(B) = 13.561d.
PT    Ser |SB, Porb = 38.937d.
del   Ser |ADS 9701A (B 5.16m, dF0, a = 5.843", Porb = 3168 yr;
del   Ser |4", 175G, 1980).
omi   Ser |SB?
d     Ser |ADS 11353 A (B 7.44m, SB?, F5V, 3.9", 320deg, 1983).
d     Ser |VB (speckle-interferometric; 0.25", 157deg, 1976).
d     Ser |SB (P1orb = 385d, P2orb = 1.8505205d).
S     Sex |P var. Max = 2422029 + 257.2d*E (JD2417650 - 22050);
S     Sex |Max = 2428968 + 266.65d*E (JD2422050 - 30300); Max =
S     Sex |2434739 + 260.86d*E (JD2430300 - 34750); Max =
S     Sex |2438796 + 254.3d*E (JD2434750 - 38800);
S     Sex |since JD2440600 - see Table.
T     Sex |[Fe/H] = -1.20. P var. Max = 2416146.675 + 0.32465971d*E
T     Sex |(JD2414000 - 18300), Max = 2424561.398 + 0.32467107d*E
T     Sex |(JD2418300 - 24570) [00752];
T     Sex |Max = 2424561.430 + 0.3246702d*E (JD2424560 - 28280),
T     Sex |Max = 2429350.320 + 0.3247113d*E (JD2429350 - 34370),
T     Sex |Max = 2434795.409 + 0.3246978d*E (JD2434795 - 36630)
T     Sex |[09978]; since JD2441380 - see Table.
U     Sex |P var. Max = 2419823.355 + 0.53402622d*E
U     Sex |(JD2419470 - 36670) [03697]; since JD2443980 - see Table.
Y     Sex |Min II 10.17; dII = 0.05P. P var. Min I = 2428122.700 +
Y     Sex |0.41982341d*E (JD < 2429000) [00007]; Min I =
Y     Sex |2434445.989 + 0.419818d*E (JD2428100 - 35000)
Y     Sex |[00001], Min I = 2439521.964 + 0.41981543d*E
Y     Sex |(JD2431150 - 43250) [09981]; since JD2440300 - see Table.
RU    Sex |Min II 11.4. According to [09923], RR?
RU    Sex |(P = 0.5398d?), CEP? (P = 6.792d?).
RW    Sex |Porb = 0.247d [09925]; LX/Lopt = 10**(-4) [09926];
RW    Sex |Px = 254s [09927].
RX    Sex |VB A (B 9.1m, 116.3", 191deg).
RY    Sex |Mu = 0.67", P = 281deg.
R     Tau |OH, H2O, Sio maser. P var. Max = 2411012 +
R     Tau |325.0d*E (JD2398654 - 2414000); Max = 2424243 +
R     Tau |322.1d*E (JD2414000 - 24300); Max = 2434005 +
R     Tau |325.4d*E (JD2424300 - 35500); since JD2435500 - see Table.
S     Tau |P var. Max = 2404646 + 380.1d*E (JD2399326 - 2405000);
S     Tau |Max = 2425085 + 371.40d*E (JD2405000 - 26000); since
S     Tau |JD2426000 - see Table.
T     Tau |VB A (B 15m, 0.27", 358deg; C - infrared companion, 0.590",
T     Tau |180deg). Near the variable nebula NGC 1555. OH, H2O maser.
T     Tau |In the interval JD2402140 - 21000 the light range
T     Tau |9.3m - 13.5m, since JD2421000 - only 9.5m - 10.8m.
U     Tau |VB (A 10.9m; B 12.0m, 3", 77deg).
V     Tau |P var. Max = 2417978 + 170.0d*E (JD2404550 - 18000);
V     Tau |Max = 2424580 + 169.3d*E (JD2418000 - 24600);
V     Tau |Max = 2432746 + 170.1d*E (JD2424600 - 33500);
V     Tau |Max = 2436970 + 168.7d*E (JD2433500 - 37300);
V     Tau |Max = 2442442 + 171.1d*E (JD2437300 - 43000);
V     Tau |since JD2443000 - see Table.
W     Tau |<P> value is given in the Table.
W     Tau |P var. Max = 2415320 + 274.1d*E (JD2410360 - 15500),
W     Tau |Max = 2421995 + 266.1d*E (JD2415500 - 22500),
W     Tau |Max = 2425135 + 260.5d*E (JD2422500 - 28800),
W     Tau |Max = 2438837 + 245.4d*E (JD2428800 - 39100) [00001].
Z     Tau |VB A (B 13.6m, 4", 45deg).
Z     Tau |P var. Max = 2425115 + 499.90d*E (JD2415100 - 26500)
Z     Tau |Max = 2438768 + 486.20d*E (JD2426500 - 39000);
Z     Tau |since JD2439000 - see Table.
RR    Tau |Spectrum description and the photographs of the nebula
RR    Tau |[04002].
RU    Tau |VB A (B 4"). P var. Max = 2426004 + 545.3d*E
RU    Tau |(JD2415009 - 27500). Max = 2434309 + 604.0d*E
RU    Tau |(JD2427500 - 34500); since JD2437500 - see Table.
RV    Tau |OH maser. Mean brightness varies: Min = 2417553 + 1224d*E
RV    Tau |[00580].
RW    Tau |VB A (12.5m, 1.3", 172deg, 1959). dI = 0.020P; Min II 8.09.
RW    Tau |P var. Min I = 2417198.410 + 2.7688665d*E +
RW    Tau |0.038d*sin(0.0818deg*(E - 100)) (JD2409913 - 24150),
RW    Tau |Min I = 2434423.3571 + 2.7688209d*E (JD2424150 - 37000)
RW    Tau |[05460]; Min I = 2437164.4860 + 2.7688480d*E
RW    Tau |(JD2437000 - 39900) [07531]; Min I = 2442776.93772 +
RW    Tau |2.76884463d*E (JD2439855 - 42780) [08593]; Min I =
RW    Tau |2442776.9313 + 2.7688396d*E (JD2442780 - 45750)
RW    Tau |[09084]; since JD2445750 - see Table. The shape of the
RW    Tau |light curve varies.
RX    Tau |OH, H2O maser. P var. Max = 2423561 + 338.4d*E
RX    Tau |(JD2417155 - 24000); Max = 2430505 + 330.2d*E
RX    Tau |(JD2424000 - 30700); Max = 2437963 + 339.3d*E
RX    Tau |(JD2430700 - 38000); since JD2438000 - see Table.
RY    Tau |SB1. The photographs of the nebula and spectrum
RY    Tau |description [05064]. Long period light variations are
RY    Tau |possible with cycles 70.25, 15.9, 9.4 and 5.84 years
RY    Tau |[09993].
RZ    Tau |Min II 10.66. P var. Min I = 2424032.1426 +
RZ    Tau |0.41567109d*E (JD2424000 - 34100) [00312];
RZ    Tau |since JD2436000 - see Table.
SS    Tau |P var [03506]. Max = 2420894.2339 + 0.3699665d*E
SS    Tau |(JD2420890 - 21300) [09995]; Max = 2426669.080 +
SS    Tau |0.3699687d*E (JD2426400 - 26700) [00320]; Max =
SS    Tau |2428843.856 + 0.3699231d*E (JD2426700 - 30300),
SS    Tau |Max = 2431392.603 + 0.369912d*E (JD2430300 - 31400),
SS    Tau |Max = 2432118.794 + 0.369937d*E (JD2431400 - 32150),
SS    Tau |Max = 2432857.884 + 0.3699146d*E (JD2432150 - 35000),
SS    Tau |Max = 2435055.528 + 0.3699066d*E (JD2435000 - 36400),
SS    Tau |Max = 2437313.503 + 0.3699266d*E (JD2436400 - 37320),
SS    Tau |Max = 2437960.419 + 0.369878d*E (JD2437300 - 37960),
SS    Tau |Max = 2437960.419 + 0.369938d*E (JD2437960 - 38740);
SS    Tau |since JD2438740 - see Table.
SV    Tau |Min II 9.8.
SW    Tau |P var. Max = 2432049.856 + 1.583623d*E (JD2418240 - 36000);
SW    Tau |since JD2436000 - see Table.
SX    Tau |In the region of the Pleiades cluster. Not a member
SX    Tau |of the cluster.
SY    Tau |In the region of the Pleiades cluster. Not a member
SY    Tau |of the cluster.
SZ    Tau |The member of the halo of the open cluster NGC 1647.
SZ    Tau |P var. Max = 2410000.60 + 3.1487d*E (JD2412000 - 20200)
SZ    Tau |[09996]; Max = 2419267.519 + 3.149046d*E
SZ    Tau |(JD2419260 - 34650); since JD2434650 - see Table.
TT    Tau |P = 364d? [00589].
TY    Tau |In the region of the hyades cluster. Not a member of
TY    Tau |the cluster. According to [09997], Min = 2422291.303 +
TY    Tau |0.539250d*E.
UU    Tau |In the region of the Pleiades cluster. Not a member of
UU    Tau |the cluster.
UX    Tau |VB A (B 13.67m V, M2.5 VE, 5.74", 270.1deg, 1944).
UZ    Tau |VB A (B 15.16m B, M4VE (Li), 3.7", 271.5deg, 1944).
UZ    Tau |The range of the combined light variation is given in the
UZ    Tau |Table.
VW    Tau |The chart in [06286] is wrong.
WW    Tau |P var. P = 114.8d (JD2414800 - 20800). P = 124.4d
WW    Tau |(JD2420800 - 23700) [00634]; P = 114d (JD2424800 - 26300),
WW    Tau |P = 139d (JD2426300 - 27700) [00310]; P = 114d
WW    Tau |(JD2427900 - 30800), P = 131d (JD2430800 - 31500),
WW    Tau |P = 109d (JD2431500 - 33400) [00364]; since
WW    Tau |JD2433400 - see Table.
WY    Tau |Min II 11.73. P var? [10048].
WZ    Tau |VB.
XZ    Tau |VB A (B = HL Tau, 23", 273deg).
YZ    Tau |[Fe/H] = -1.53. In the region of the Pleiades cluster.
YZ    Tau |Not a member of the cluster.
YZ    Tau |There is a square term in the elements: -6d*10**(-11)*E**2.
AA    Tau |Cyclic light variation with P = 4.5d and 2d [10003] and
AA    Tau |also 8.2d [10004] is possible.
AC    Tau |d = 0.025P. P var?
AH    Tau |Min II 11.85. P var? In the region of the Pleiades
AH    Tau |cluster. Not a member of the cluster.
AL    Tau |P var. The depth of Min II 0.15m.
AM    Tau |d = 0.012P:. P var. Min I = 2427534.444 + 2.044018d*E
AM    Tau |(JD2425580 - 27540), Min I = 2435019.436 +
AM    Tau |2.043935d*E (JD2433320 - 37020); since JD2442365 - see
AM    Tau |Table.
AN    Tau |Min II 10.5; Min II - Min I = 0.53P. P var.
AP    Tau |Min II 14.7; Min II - Min I = 0.48P.
AS    Tau |P var. Min I = 2439390.595 + 3.4835542d*E
AS    Tau |(JD2419440 - 44300) [07806]; since JD2444300 - see Table.
AU    Tau |P var. Max = 2426642 + 71.0d*E (JD2426290 - 30400)
AU    Tau |[00310]; since JD2438000 - see Table.
AW    Tau |OH, H2O maser. P var. Max = 2426278 + 690d*E
AW    Tau |(JD2416100 - 33850) [00609]; since JD2433850 - see Table.
BB    Tau |SC 7/7 e.
BK    Tau |In the region of the Pleiades cluster. Not a member of
BK    Tau |the cluster.
BN    Tau |P var. Min I = 2435460.370 + 4.2542044d*E
BN    Tau |(JD2419000-39100) [05466]; since JD2443000 - see Table.
BP    Tau |There are quasisinusoidal light variations with P = 7.6d
BP    Tau |[10011].
BU    Tau |Pleione. The member of the Pleiades cluster.
BV    Tau |Min II 11.9.
BW    Tau |3C 120. Seyfert galaxy; Z = 0.033. Spectrum description
BW    Tau |[10012].
CD    Tau |VB A (B 9.88m, 9.9", 148.8deg). Min II 7.31.
CD    Tau |In the region of the open cluster CR 65.
CF    Tau |d = 0.02P; Min II 10.2;
CH    Tau |The epoch of Min brightness is given.
CM    Tau |SN 1054 in the Crab nebula (NGC 1952 = M1); pulsar NP 0532.
CM    Tau |The outburst epoch is JD2106210:. The pulsed radiation
CM    Tau |varies precisely in phase over the whole spectrum, from
CM    Tau |radio waves to gamma rays with P = 0.033S in the range
CM    Tau |13.9m - 17.7m V. P var [10017,10018]: 0.033095563927s
CM    Tau |(JD2440297.5094) <= P <= 0.033242051159s (JD2444312.750).
CR    Tau |P = 1.362692d?
CT    Tau |Min II 11.12. P var. Min I = 2437312.369 + 0.6668274d*E
CT    Tau |(JD2432700 - 38790) [10010]; since JD2441400 - see Table.
CU    Tau |In the region of the Pleiades cluster. Not a member of
CU    Tau |the cluster. Min II 11.90. P var. Min I =
CU    Tau |2431822.5193 + 0.4126022d*E (JD2431060 - 2890)
CU    Tau |[00604]; since JD2440960 - see Table.
CZ    Tau |VB B (A = DD Tau; B 31", 13deg).
DD    Tau |VB A (B = CZ Tau; 31", 13deg.
DE    Tau |VB A (B 26", 10deg).
DG    Tau |Connected with a small bright arc-shaped nebula.
DH    Tau |VB A (B = DI Tau, 16", 125deg). According to [10004] there
DH    Tau |is periodical light variability with P = 7.0d and
DH    Tau |A = 0.4m V.
DI    Tau |VB B (A = DH Tau; B 16", 125deg).
DI    Tau |According to [10004] there is
DI    Tau |periodical light variability with P ~7.0d and A < 0.4m V.
DL    Tau |VB A (B 17m V, 12", 333deg).
DL    Tau |Cyclic light variation with P = 2.7d is present [10003].
DN    Tau |There are sinusoidal light variations with
DN    Tau |P = 6.6d [10011].
DO    Tau |Connected with a small bright arc-shaped nebula.
DS    Tau |VB A (B 13.7m, 4", 288deg). Range of Combined light
DS    Tau |variation of the pair is given in the Table.
EI    Tau |VB?
EQ    Tau |Min II 10.97. In the region of the Pleiades cluster.
EQ    Tau |Not a member of the cluster.
ES    Tau |Min II 14.4; Min II - Min I = 0.52P; d = 0.005P.
ET    Tau |Min II 9.3.
EY    Tau |The member of the Hyades cluster.
EZ    Tau |The member of the Hyades cluster.
FH    Tau |The member of the Hyades cluster.
FL    Tau |The member of the Pleiades cluster.
FS    Tau |VB A (B 16", 289deg).
FV    Tau |VB A (B 13", 103deg).
FW    Tau |VB A (B 13", 243deg).
FY    Tau |VB B (A = FZ Tau, B 17", 250deg.)
FZ    Tau |VB A (B = FY Tau, 17", 250deg).
GG    Tau |VB A (B 18.5m, 12", 205deg).
GH    Tau |VB B (A = V807 Tau; B 21.4", 193deg).
GI    Tau |VB B (A = GK Tau; B 13", 329deg). There are
GI    Tau |quasisinusoidal light variations with P = 7.2d [10011].
GI    Tau |Connected with a small bright arc-shaped nebula.
GK    Tau |VB A (B = GI Tau, 13", 329deg).
GK    Tau |There are quasisinusoidal light variations with P = 4.6d
GK    Tau |[10011]. Connected with a small bright arc-shaped nebula.
GL    Tau |The central star of the planetary nebula PK 174 -14deg 1.
GP    Tau |P2 = 1000d.
GR    Tau |dI = 0.068P; Min II 10.49; Mim II - Min I = 0.516P.
GS    Tau |SB1 (Porb = 7.227424d [06568]). The epoch of Min
GS    Tau |brightness is given.
GU    Tau |VB A (B 11", 299deg).
GV    Tau |Herbig-haro object.
GW    Tau |Min II 11.7. P var?
GX    Tau |VB A (B 11", 310deg).
HK    Tau |VB A (B 21m, 2", 180deg).
HL    Tau |VB B (A = XZ Tau; B 23", 273deg). Connected with a
HL    Tau |small bright arc-shaped nebula.
HN    Tau |VB A (B 18m, 3.3", 205deg).
HO    Tau |VB A (B 8", 110deg).
HP    Tau |Connected with a small bright arc-shaped nebula.
HP    Tau |According to [10004] there is periodical variability
HP    Tau |with P = 1.2d.
HR    Tau |VB B (A = HS Tau; B 14", 119deg).
HS    Tau |VB A (B = HR Tau; 14", 119deg).
HU    Tau |Min II 5.91.
HW    Tau |Minor planet (49) Pales.
HZ    Tau |In the region of the Pleiades cluster. Possible
HZ    Tau |member of the cluster.
II    Tau |In the region of the Pleiades cluster.
II    Tau |Possible member of the hyades cluster
IK    Tau |OH, H2O, SiO maser.
IM    Tau |P var. Max = 2439792.398 + 0.144969d*E (JD2439790 -
IM    Tau |43130) [10019]; P1 = 0.109016d, P1/P0 = 0.752.
IM    Tau |Since JD2444230 - see Table.
IN    Tau |mu = 0.121", P = 105deg. The member of the Hyades cluster?
IO    Tau |In the region of the Hyades cluster.
IQ    Tau |VB A (B 17m, 11", 298deg).
IS    Tau |SVS 1319 [04051].
IS    Tau |The star N23 with Halpha emission [00596]. In the map given
IS    Tau |in [00596] erroneously designated as N26 in contradiction
IS    Tau |with the co-ordinates given in the same paper. It was the
IS    Tau |reason for different mistakes when the
IS    Tau |star was identified by some other investigators.
IT    Tau |SVS 1320 [04051].
IT    Tau |The star N26 with Halpha emission [00596].
IT    Tau |In the map given in [00596] IS Tau erroneously designated
IT    Tau |as N26 in contradiction with the co-ordinates given in the
IT    Tau |same paper. It was the reason for different mistakes when
IT    Tau |IS Tau was identified by some other investigators.
KK    Tau |In the region of the Pleiades cluster.
KL    Tau |In the region of the Pleiades cluster.
KM    Tau |In the region of the Pleiades cluster.
KN    Tau |In the region of the Pleiades cluster.
KO    Tau |In the region of the Pleiades cluster.
KP    Tau |In the region of the Pleiades cluster. Not a member
KP    Tau |of the cluster.
KQ    Tau |In the region of the Pleiades cluster.
KR    Tau |In the region of the Pleiades cluster. Not a member
KR    Tau |of the cluster.
KS    Tau |In the region of the Pleiades cluster.
KT    Tau |In the region of the Pleiades cluster.
KU    Tau |In the region of the Pleiades cluster.
KV    Tau |In the region of the Pleiades cluster.
KW    Tau |In the region of the Pleiades cluster.
KX    Tau |In the region of the Pleiades cluster. Not a member
KX    Tau |of the cluster.
KY    Tau |The member of the Pleiades cluster.
KZ    Tau |In the region of the Pleiades cluster.
LL    Tau |In the region of the Pleiades cluster.
LM    Tau |In the region of the Pleiades cluster. Possible member
LM    Tau |of the cluster.
LN    Tau |In the region of the Pleiades cluster.
LO    Tau |In the region of the Pleiades cluster. Possible member
LO    Tau |of the cluster.
LP    Tau |In the region of the Pleiades cluster. Not a member
LP    Tau |of the cluster.
LQ    Tau |In the region of the Pleiades cluster.
LR    Tau |In the region of the Pleiades cluster. Possible member
LR    Tau |of the Hyades cluster.
LS    Tau |In the region of the Pleiades cluster.
LT    Tau |In the region of the Pleiades cluster. Possible member
LT    Tau |of the cluster.
LU    Tau |In the region of the Pleiades cluster. Possible member
LU    Tau |of the cluster.
LV    Tau |In the region of the Pleiades cluster. Possible member
LV    Tau |of the cluster.
LW    Tau |In the region of the Pleiades cluster. Not a member
LW    Tau |of the cluster.
LX    Tau |In the region of the Pleiades cluster.
LY    Tau |In the region of the Pleiades cluster. Possible member
LY    Tau |of the cluster.
LZ    Tau |The member of the Pleiades cluster.
MM    Tau |The member of the Pleiades cluster.
MN    Tau |In the region of the Pleiades cluster.
MO    Tau |In the region of the Pleiades cluster. Possible member
MO    Tau |of the cluster.
MP    Tau |In the region of the Pleiades cluster.
MQ    Tau |In the region of the Pleiades cluster.
MR    Tau |The member of the Pleiades cluster.
MS    Tau |The member of the Pleiades cluster.
MT    Tau |In the region of the Pleiades cluster. Not a member
MT    Tau |of the  cluster.
MU    Tau |In the region of the Pleiades cluster. Possible member
MU    Tau |of the cluster.
MV    Tau |In the region of the Pleiades cluster. Possible member
MV    Tau |of the cluster.
MW    Tau |In the region of the Pleiades cluster.
MX    Tau |The member of the Pleiades cluster.
MY    Tau |The member of the Pleiades cluster.
MZ    Tau |In the region of the Pleiades cluster. Possible member
MZ    Tau |of the cluster.
NN    Tau |In the region of the Pleiades cluster.
NO    Tau |In the region of the Pleiades cluster.
NP    Tau |The member of the Pleiades cluster.
NQ    Tau |In the region of the Pleiades cluster.
NR    Tau |In the region of the Pleiades cluster. Not a member
NR    Tau |of the cluster.
NS    Tau |In the region of the Pleiades cluster.
NT    Tau |In the region of the Pleiades cluster. Possible member
NT    Tau |of the cluster.
NU    Tau |In the region of the Pleiades cluster.
NV    Tau |In the region of the Pleiades cluster. Not a member
NV    Tau |of the cluster.
NW    Tau |In the region of the Pleiades cluster.
NX    Tau |In the region of the Pleiades cluster. Not a member
NX    Tau |of the cluster.
NY    Tau |In the region of the Pleiades cluster. Not a member
NY    Tau |of the cluster.
NZ    Tau |In the region of the Pleiades cluster.
OO    Tau |In the region of the Pleiades cluster.
OP    Tau |In the region of the Pleiades cluster. Possible member
OP    Tau |of the cluster.
OQ    Tau |In the region of the Pleiades cluster.
OR    Tau |The member of the Pleiades cluster.
OS    Tau |The member of the Pleiades cluster.
OT    Tau |The member of the Pleiades cluster.
OU    Tau |Max = 2444896.758 + 0.39701d*E, M - m = 0.5P, A(V) =
OU    Tau |0.13m [10052].
OU    Tau |The member of the Pleiades cluster.
OW    Tau |The member of the Pleiades cluster.
OX    Tau |In the region of the Pleiades cluster.
OY    Tau |In the region of the Pleiades cluster. Not a member
OY    Tau |of the cluster.
OZ    Tau |In the region of the Pleiades cluster. Possible member
OZ    Tau |of the cluster.
PP    Tau |In the region of the Pleiades cluster. Possible member
PP    Tau |of the cluster.
PQ    Tau |In the region of the Pleiades cluster. Not a member
PQ    Tau |of the cluster.
PR    Tau |The member of the Pleiades cluster.
PS    Tau |In the region of the Pleiades cluster.
PT    Tau |The member of the Pleiades cluster.
PU    Tau |In the region of the Pleiades cluster.
PV    Tau |In the region of the Pleiades cluster. Possible member
PV    Tau |of the cluster.
PW    Tau |In the region of the Pleiades cluster.
PZ    Tau |In the region of the Pleiades cluster.
QQ    Tau |SB2. The member of the Pleiades cluster.
QR    Tau |In the region of the Pleiades cluster.
QS    Tau |In the region of the Pleiades cluster.
QT    Tau |In the region of the Pleiades cluster.
QU    Tau |VB A (B 18.0m, 4.0", 135deg). In the region of the
QU    Tau |Pleiades cluster.
QV    Tau |In the region of the Pleiades cluster.
QW    Tau |In the region of the Pleiades cluster.
QX    Tau |The member of the Pleiades cluster.
QX    Tau |Max = 2444896.79 + 0.483d*E, M - m = 0.5P, A(V) = 0.125m
QX    Tau |[10052].
QY    Tau |In the region of the Pleiades cluster. Not a member
QY    Tau |of the cluster.
QZ    Tau |In the region of the Pleiades cluster.
V0335 Tau |In the region of the Pleiades cluster.
V0336 Tau |In the region of the Pleiades cluster. Possible member
V0336 Tau |of the cluster.
V0337 Tau |In the region of the Pleiades cluster.
V0338 Tau |In the region of the Pleiades cluster. Possible member
V0338 Tau |of the cluster.
V0339 Tau |In the region of the Pleiades cluster. Not a member
V0339 Tau |of the cluster.
V0340 Tau |In the region of the Pleiades cluster.
V0341 Tau |In the region of the Pleiades cluster.
V0342 Tau |In the region of the Pleiades cluster.
V0343 Tau |The member of the Pleiades cluster.
V0344 Tau |In the region of the Pleiades cluster.
V0345 Tau |In the region of the Pleiades cluster.
V0346 Tau |The member of the Pleiades cluster.
V0347 Tau |In the region of the Pleiades cluster. Not a member
V0347 Tau |of the cluster.
V0348 Tau |In the region of the Pleiades cluster.
V0349 Tau |In the region of the Pleiades cluster. Possible member
V0349 Tau |of the cluster.
V0350 Tau |In the region of the Pleiades cluster. Possible member
V0350 Tau |of the cluster.
V0351 Tau |In the region of the Pleiades cluster. Not a member
V0351 Tau |of the cluster.
V0352 Tau |In the region of the Pleiades cluster.
V0353 Tau |In the region of the Pleiades cluster. Possible member
V0353 Tau |of the cluster.
V0354 Tau |In the region of the Pleiades cluster. Possible member
V0354 Tau |of the cluster.
V0355 Tau |In the region of the Pleiades cluster. Possible member
V0355 Tau |of the cluster.
V0356 Tau |In the region of the Pleiades cluster.
V0357 Tau |The member of the Pleiades cluster.
V0358 Tau |The member of the Pleiades cluster.
V0359 Tau |In the region of the Pleiades cluster.
V0360 Tau |In the region of the Pleiades cluster.
V0361 Tau |In the region of the Pleiades cluster. Possible member
V0361 Tau |of the cluster.
V0362 Tau |In the region of the Pleiades cluster.
V0363 Tau |In the region of the Pleiades cluster. Possible member
V0364 Tau |In the region of the Pleiades cluster. Possible member
V0364 Tau |of the cluster.
V0365 Tau |In the region of the Pleiades cluster.
V0366 Tau |The member of the Pleiades cluster.
V0367 Tau |In the region of the Pleiades cluster.
V0368 Tau |In the region of the Pleiades cluster.
V0369 Tau |In the region of the Pleiades cluster.
V0370 Tau |The member of the Pleiades cluster.
V0371 Tau |VB (Delta(m) ~1m, 1.5"). The member of the Pleiades
V0371 Tau |cluster.
V0372 Tau |The member of the Pleiades cluster.
V0373 Tau |In the region of the Pleiades cluster.
V0374 Tau |In the region of the Pleiades cluster.
V0375 Tau |In the region of the Pleiades cluster. Not a member
V0375 Tau |of the cluster.
V0376 Tau |The member of the Pleiades cluster.
V0377 Tau |The member of the Pleiades cluster.
V0378 Tau |The member of the Pleiades cluster.
V0379 Tau |In the region of the Pleiades cluster. Possible member
V0379 Tau |of the cluster.
V0380 Tau |In the region of the Pleiades cluster. Possible member
V0380 Tau |of the cluster.
V0381 Tau |The member of the Pleiades cluster.
V0382 Tau |The member of the Pleiades cluster.
V0383 Tau |In the region of the Pleiades cluster.
V0384 Tau |The member of the Pleiades cluster.
V0385 Tau |In the region of the Pleiades cluster. Not a member
V0385 Tau |of the cluster.
V0386 Tau |TCSN 437. In the region of the Pleiades cluster.
V0387 Tau |In the region of the Pleiades cluster.
V0388 Tau |In the region of the Pleiades cluster.
V0389 Tau |TCSN 439. In the region of the Pleiades cluster.
V0390 Tau |In the region of the Pleiades cluster.
V0392 Tau |In the region of the Pleiades cluster. Possible member
V0392 Tau |of the cluster.
V0394 Tau |In the region of the Pleiades cluster. Not a member
V0394 Tau |of the cluster.
V0395 Tau |In the region of the Pleiades cluster.
V0396 Tau |In the region of the Pleiades cluster.
V0397 Tau |In the region of the Pleiades cluster.
V0398 Tau |In the region of the Pleiades cluster. Possible member
V0398 Tau |of the cluster.
V0399 Tau |The member of the Pleiades cluster.
V0400 Tau |In the region of the Pleiades cluster.
V0401 Tau |In the region of the Pleiades cluster.
V0402 Tau |The member of the Pleiades cluster.
V0403 Tau |The member of the Pleiades cluster.
V0404 Tau |In the region of the Pleiades cluster.
V0405 Tau |In the region of the Pleiades cluster.
V0410 Tau |There are periodical light variations with P = 1.92d,
V0410 Tau |A(V) = 0.21m, M - m = 0.5P [10056].
V0411 Tau |mu = 0.13", P = 143deg.
V0411 Tau |Eruptive white dwarf. Usually there are quasi-perio-
V0411 Tau |dic variations with A ~0.3m and periods P0 = 12.436
V0411 Tau |Min and P1 = 8.237 Min (P1/P0 = 0.6624) which are
V0411 Tau |nonlinearly modulated by the third period PL ~0.135d
V0411 Tau |(probably by the orbital period of a faint companion).
V0421 Tau |Minor planet (586) Thekla.
V0423 Tau |Min II 15.8.
V0425 Tau |In the region of the Pleiades cluster. Not a member
V0425 Tau |of the cluster.
V0426 Tau |In the region of the Pleiades cluster.
V0427 Tau |In the region of the Pleiades cluster.
V0428 Tau |In the region of the Pleiades cluster.
V0429 Tau |In the region of the Pleiades cluster.
V0430 Tau |In the region of the Pleiades cluster. Possible member
V0430 Tau |of the cluster.
V0431 Tau |In the region of the Pleiades cluster.
V0432 Tau |In the region of the Pleiades cluster.
V0433 Tau |In the region of the Pleiades cluster.
V0434 Tau |In the region of the Pleiades cluster.
V0435 Tau |In the region of the Pleiades cluster. Possible member
V0435 Tau |of the cluster.
V0436 Tau |In the region of the Pleiades cluster. Not a member
V0436 Tau |of the cluster.
V0437 Tau |In the region of the Pleiades cluster. Not a member
V0437 Tau |of the cluster.
V0438 Tau |In the region of the Pleiades cluster. Possible member
V0438 Tau |of the cluster.
V0439 Tau |In the region of the Pleiades cluster.
V0440 Tau |In the region of the Pleiades cluster.
V0441 Tau |In the region of the Pleiades cluster. Possible member
V0441 Tau |of the cluster.
V0442 Tau |In the region of the Pleiades cluster.
V0443 Tau |In the region of the Pleiades cluster.
V0444 Tau |In the region of the Pleiades cluster. Possible member
V0444 Tau |of the cluster.
V0445 Tau |In the region of the Pleiades cluster.
V0446 Tau |The member of the Pleiades cluster.
V0447 Tau |In the region of the Pleiades cluster. Not a member
V0447 Tau |of the cluster.
V0448 Tau |The member of the Pleiades cluster.
V0449 Tau |In the region of the Pleiades cluster. Not a member
V0449 Tau |of the cluster.
V0451 Tau |In the region of the Pleiades cluster. Not a member
V0451 Tau |of the cluster.
V0452 Tau |In the region of the Pleiades cluster. Possible member
V0452 Tau |of the cluster.
V0453 Tau |In the region of the Pleiades cluster. Possible member
V0453 Tau |of the cluster.
V0454 Tau |In the region of the Pleiades cluster. Not a member
V0454 Tau |of the cluster.
V0455 Tau |In the region of the Pleiades cluster.
V0456 Tau |In the region of the Pleiades cluster.
V0457 Tau |In the region of the Pleiades cluster.
V0458 Tau |In the region of the Pleiades cluster.
V0459 Tau |In the region of the Pleiades cluster.
V0460 Tau |In the region of the Pleiades cluster.
V0461 Tau |In the region of the Pleiades cluster. Possible member
V0461 Tau |of the cluster.
V0462 Tau |In the region of the Pleiades cluster. Not a member
V0462 Tau |of the cluster.
V0463 Tau |In the region of the Pleiades cluster.
V0464 Tau |In the region of the Pleiades cluster.
V0465 Tau |In the region of the Pleiades cluster.
V0466 Tau |In the region of the Pleiades cluster. Possible member
V0466 Tau |of the cluster.
V0467 Tau |In the region of the Pleiades cluster.
V0468 Tau |In the region of the Pleiades cluster.
V0469 Tau |In the region of the Pleiades cluster.
V0470 Tau |In the region of the Pleiades cluster. Possible member
V0470 Tau |of the cluster.
V0471 Tau |The member of the Hyades cluster. mu alpha =  + 0.117",
V0471 Tau |mu delta = -0.020".
V0471 Tau |EA/D/(RS + WD) + XP. d = 0.0625P.
V0471 Tau |There occurs a total eclipse of the white dwarf in
V0471 Tau |Min I (A = 0.04m V, 0.36m U).
V0471 Tau |P var. Min I = 2440612.67083 + 0.52118321d*E
V0471 Tau |(JD2440570 - 970) [06250]; Min I = 2440898.80038 +
V0471 Tau |0.52118376d*E (JD2440880 - 41360), Min I =
V0471 Tau |2441665.46153 + 0.52118329d*E (JD2441660 -
V0471 Tau |42100) [10058]; since JD2441900 - see Table.
V0471 Tau |Wave-like distorsion with the amplitude from 0.05m
V0471 Tau |up to 0.27m and with the period close to the orbital
V0471 Tau |one is observed in the light curve outside eclipses;
V0471 Tau |sometimes there are also flares. The wave is migrating on
V0471 Tau |phase in the direction of phase decreasing
V0471 Tau |with a migration period of 191d [10060] or ~250d
V0471 Tau |[10061]. The period of white dwarf rotation derived
V0471 Tau |through X-ray observations Ppuls = 554.73s [10062].
V0472 Tau |In the region of the Pleiades cluster.
V0473 Tau |P = 2.7800d?
V0474 Tau |In the region of the Pleiades cluster. Not a member
V0474 Tau |of the cluster.
V0475 Tau |In the region of the Pleiades cluster.
V0476 Tau |In the region of the Pleiades cluster.
V0477 Tau |In the region of the Pleiades cluster.
V0478 Tau |In the region of the Pleiades cluster.
V0479 Tau |VB A (BC 8.90m, 59", 357deg); (k - b)2 = 0.40.
V0480 Tau |VB A (B 10.4m, 176", 303deg). The member of the Hyades
V0480 Tau |cluster.
V0481 Tau |In the region of the Pleiades cluster.
V0483 Tau |The member of the Hyades cluster.
V0484 Tau |The member of the Hyades cluster.
V0485 Tau |In the region of the Pleiades cluster.
V0486 Tau |Epoch of Max (U) is given.
V0486 Tau |P =/ 10.61d? [10063].
V0487 Tau |In the region of the Pleiades cluster. Not a member
V0487 Tau |of the cluster.
V0487 Tau |On the photograph west is at the top and
V0487 Tau |south to the right.
V0488 Tau |The member of the Pleiades cluster.
V0489 Tau |In the region of the Pleiades cluster.
V0490 Tau |In the region of the Pleiades cluster.
V0491 Tau |In the region of the Pleiades cluster. Possible member
V0491 Tau |of the cluster.
V0492 Tau |In the region of the Pleiades cluster. Possible member
V0492 Tau |of the cluster.
V0493 Tau |In the region of the Pleiades cluster.
V0494 Tau |In the region of the Pleiades cluster. Not a member
V0494 Tau |of the cluster.
V0495 Tau |In the region of the Pleiades cluster.
V0496 Tau |In the region of the Pleiades cluster.
V0497 Tau |In the region of the Pleiades cluster. Possible member
V0497 Tau |of the cluster.
V0498 Tau |In the region of the Pleiades cluster. Not a member
V0498 Tau |of the cluster.
V0499 Tau |In the region of the Pleiades cluster.
V0500 Tau |The member of the Pleiades cluster.
V0501 Tau |In the region of the Pleiades cluster. Not a member
V0501 Tau |of the cluster.
V0502 Tau |The member of the Pleiades cluster.
V0503 Tau |In the region of the Pleiades cluster. Not a member
V0503 Tau |of the cluster.
V0504 Tau |In the region of the Pleiades cluster.
V0506 Tau |In the region of the Pleiades cluster. Not a member
V0506 Tau |of the cluster.
V0507 Tau |In the region of the Pleiades cluster.
V0508 Tau |In the region of the Pleiades cluster.
V0509 Tau |In the region of the Pleiades cluster.
V0510 Tau |In the region of the Pleiades cluster.
V0511 Tau |In the region of the Pleiades cluster.
V0512 Tau |In the region of the Pleiades cluster.
V0513 Tau |In the region of the Pleiades cluster.
V0514 Tau |In the region of the Pleiades cluster.
V0515 Tau |In the region of the Pleiades cluster.
V0516 Tau |In the region of the Pleiades cluster.
V0517 Tau |In the region of the Pleiades cluster. Not a member
V0517 Tau |of the cluster.
V0518 Tau |VB B (A 14.4m; B 10", 80deg). The member of the
V0518 Tau |Pleiades cluster.
V0519 Tau |In the region of the Pleiades cluster. Not a member
V0519 Tau |of the cluster.
V0520 Tau |In the region of the Pleiades cluster. Possible member
V0520 Tau |of the cluster.
V0521 Tau |In the region of the Pleiades cluster. Not a member
V0521 Tau |of the cluster.
V0522 Tau |In the region of the Pleiades cluster.
V0523 Tau |In the region of the Pleiades cluster. Not a member
V0523 Tau |of the cluster.
V0524 Tau |In the region of the Pleiades cluster.
V0525 Tau |In the region of the Pleiades cluster. Not a member
V0525 Tau |of the cluster.
V0526 Tau |In the region of the Pleiades cluster.
V0527 Tau |In the region of the Pleiades cluster. Not a member
V0527 Tau |of the cluster.
V0528 Tau |In the region of the Pleiades cluster.
V0529 Tau |In the region of the Pleiades cluster. Not a member
V0529 Tau |of the cluster.
V0530 Tau |In the region of the Pleiades cluster. Not a member
V0530 Tau |of the cluster.
V0531 Tau |In the region of the Pleiades cluster.
V0532 Tau |In the region of the Pleiades cluster.
V0533 Tau |In the region of the Pleiades cluster.
V0534 Tau |In the region of the Pleiades cluster.
V0535 Tau |In the region of the Pleiades cluster.
V0536 Tau |In the region of the Pleiades cluster.
V0537 Tau |In the region of the Pleiades cluster.
V0538 Tau |The member of the Pleiadea cluster.
V0539 Tau |In the region of the Pleiades cluster. Possible member
V0539 Tau |of the cluster.
V0540 Tau |The member of the Pleiades cluster.
V0541 Tau |The member of the Pleiades cluster.
V0542 Tau |In the region of the Pleiades cluster. Not a member
V0542 Tau |of the cluster.
V0543 Tau |In the region of the Pleiades cluster.
V0544 Tau |In the region of the Pleiades cluster.
V0545 Tau |Max = 2444896.678 + 0.355d*E, M - m = 0.42P, A(V) =
V0545 Tau |0.09m [10052]. The member of the Pleiades cluster.
V0546 Tau |In the region of the Pleiades cluster. Not a member
V0546 Tau |of the cluster.
V0547 Tau |In the region of the Pleiades cluster.
V0548 Tau |In the region of the Pleiades cluster. Possible member
V0548 Tau |of the cluster.
V0549 Tau |In the region of the Pleiades cluster.
V0550 Tau |The member of the Pleiades cluster.
V0551 Tau |In the region of the Pleiades cluster.
V0552 Tau |In the region of the Pleiades cluster.
V0553 Tau |In the region of the Pleiades cluster. Not a member
V0553 Tau |of the cluster.
V0554 Tau |In the region of the Pleiades cluster.
V0555 Tau |In the region of the Pleiades cluster. Not a member
V0555 Tau |of the cluster.
V0556 Tau |In the region of the Pleiades cluster.
V0557 Tau |In the region of the Pleiades cluster. Not a member
V0557 Tau |of the cluster.
V0558 Tau |In the region of the Pleiades cluster.
V0559 Tau |In the region of the Pleiades cluster. Not a member
V0559 Tau |of the cluster.
V0560 Tau |In the region of the Pleiades cluster. Not a member
V0560 Tau |of the cluster.
V0561 Tau |In the region of the Pleiades cluster.
V0562 Tau |In the region of the Pleiades cluster.
V0563 Tau |In the region of the Pleiades cluster.
V0564 Tau |In the region of the Pleiades cluster.
V0565 Tau |In the region of the Pleiades cluster. Not a member
V0565 Tau |of the cluster.
V0566 Tau |In the region of the Pleiades cluster. Not a member
V0566 Tau |of the cluster.
V0567 Tau |In the region of the Pleiades cluster.
V0568 Tau |In the region of the Pleiades cluster.
V0569 Tau |In the region of the Pleiades cluster. Not a member
V0569 Tau |of the cluster.
V0570 Tau |In the region of the Pleiades cluster.
V0571 Tau |In the region of the Pleiades cluster.
V0572 Tau |In the region of the Pleiades cluster.
V0573 Tau |In the region of the Pleiades cluster.
V0574 Tau |In the region of the Pleiades cluster.
V0575 Tau |In the region of the Pleiades cluster.
V0576 Tau |In the region of the Pleiades cluster.
V0577 Tau |In the region of the Pleiades cluster.
V0578 Tau |In the region of the Pleiades cluster. Not a member
V0578 Tau |of the cluster.
V0579 Tau |In the region of the Pleiades cluster.
V0581 Tau |In the region of the Pleiades cluster.
V0582 Tau |In the region of the Pleiades cluster.
V0583 Tau |In the region of the Pleiades cluster.
V0584 Tau |In the region of the Pleiades cluster.
V0585 Tau |In the region of the Hyades cluster.
V0589 Tau |In the region of the Hyades cluster.
V0594 Tau |In the region of the Pleiades cluster.
V0595 Tau |In the region of the Pleiades cluster.
V0596 Tau |In the region of the Pleiades cluster. Possible member
V0596 Tau |of the cluster.
V0597 Tau |In the region of the Pleiades cluster.
V0598 Tau |In the region of the Pleiades cluster.
V0599 Tau |In the region of the Pleiades cluster.
V0600 Tau |In the region of the Pleiades cluster.
V0601 Tau |In the region of the Pleiades cluster.
V0602 Tau |In the region of the Pleiades cluster. Not a member
V0602 Tau |of the cluster.
V0603 Tau |In the region of the Pleiades cluster.
V0604 Tau |In the region of the Pleiades cluster.
V0605 Tau |In the region of the Pleiades cluster.
V0606 Tau |In the region of the Pleiades cluster.
V0607 Tau |In the region of the Pleiades cluster.
V0608 Tau |In the region of the Pleiades cluster. Not a member
V0608 Tau |of the cluster.
V0609 Tau |In the region of the Pleiades cluster.
V0610 Tau |The member of the Pleiades cluster.
V0611 Tau |In the region of the Pleiades cluster.
V0612 Tau |In the region of the Pleiades cluster.
V0613 Tau |In the region of the Pleiades cluster. Possible member
V0613 Tau |of the cluster.
V0614 Tau |In the region of the Pleiades cluster.
V0615 Tau |In the region of the Pleiades cluster. Not a member
V0615 Tau |of the cluster.
V0617 Tau |In the region of the Pleiades cluster.
V0618 Tau |In the region of the Pleiades cluster.
V0619 Tau |In the region of the Pleiades cluster.
V0620 Tau |In the region of the Pleiades cluster.
V0621 Tau |In the region of the Pleiades cluster.
V0622 Tau |In the region of the Pleiades cluster.
V0623 Tau |The member of the Pleiades cluster.
V0624 Tau |The value of P1(A1 = 0.01m) is given in the Table.
V0624 Tau |P2 = 0.017d, A2 = 0.007m. The member of the Pleiades
V0624 Tau |cluster.
V0625 Tau |In the region of the Pleiades cluster.
V0626 Tau |In the region of the Pleiades cluster.
V0627 Tau |The member of the Pleiades cluster.
V0629 Tau |In the region of the Pleiades cluster.
V0630 Tau |In the region of the Pleiades cluster.
V0631 Tau |The member of the Pleiades cluster.
V0632 Tau |The member of the Pleiades cluster.
V0633 Tau |In the region of the Pleiades cluster. Not a member
V0633 Tau |of the cluster.
V0634 Tau |In the region of the Pleiades cluster. Not a member
V0634 Tau |of the cluster.
V0635 Tau |The member of the Pleiades cluster.
V0636 Tau |In the region of the Pleiades cluster. Not a member
V0636 Tau |of the cluster.
V0637 Tau |In the region of the Pleiades cluster.
V0638 Tau |The member of the Pleiades cluster.
V0639 Tau |In the region of the Pleiades cluster.
V0640 Tau |In the region of the Pleiades cluster.
V0641 Tau |Max = 2444896.744 + 1.22d*E; M - m = 0.5P, A(V) = 0.03m
V0641 Tau |[10052]. The member of the Pleiades cluster.
V0642 Tau |The member of the Pleiades cluster.
V0643 Tau |The member of the Pleiades cluster.
V0644 Tau |The member of the Pleiades cluster.
V0645 Tau |In the region of the Pleiades cluster. Possible member
V0645 Tau |of the cluster.
V0646 Tau |The member of the Pleiades cluster.
V0647 Tau |The value
V0647 Tau |of P1(A1 = 0.011m) is given in the Table.
V0647 Tau |P2 = 0.070d, A2 = 0.006m. The member of the Pleiades
V0647 Tau |cluster.
V0648 Tau |In the region of the Pleiades cluster.
V0649 Tau |In the region of the Pleiades cluster.
V0650 Tau |The member of the Pleiades cluster.
V0651 Tau |In the region of the Pleiades cluster.
V0652 Tau |The member of the Pleiades cluster.
V0653 Tau |In the region of the Pleiades cluster. Not a member
V0653 Tau |of the cluster.
V0654 Tau |In the region of the Pleiades cluster. Possible member
V0654 Tau |of the cluster.
V0655 Tau |In the region of the Pleiades cluster.
V0656 Tau |In the region of the Pleiades cluster.
V0657 Tau |In the region of the Pleiades cluster. Not a member
V0657 Tau |of the cluster.
V0658 Tau |In the region of the Pleiades cluster.
V0659 Tau |In the region of the Pleiades cluster.
V0660 Tau |Max = 2444896.453 + 0.23541d*E, M - m = 0.5P, A(V) =
V0660 Tau |0.20m [10052]. The member of the Pleiades cluster.
V0661 Tau |In the region of the Pleiades cluster.
V0662 Tau |In the region of the Pleiades cluster.
V0663 Tau |In the region of the Pleiades cluster.
V0664 Tau |The member of the Pleiades cluster.
V0665 Tau |In the region of the Pleiades cluster. Not a member
V0665 Tau |of the region.
V0666 Tau |In the region of the Pleiades cluster.
V0667 Tau |The member of the Pleiades cluster.
V0668 Tau |In the region of the Pleiades cluster.
V0669 Tau |In the region of the Pleiades cluster.
V0670 Tau |In the region of the Pleiades cluster.
V0671 Tau |In the region of the Pleiades cluster.
V0672 Tau |In the region of the Pleiades cluster. Not a member
V0672 Tau |of the cluster.
V0673 Tau |In the region of the Pleiades cluster. Possible member
V0673 Tau |of the cluster.
V0674 Tau |In the region of the Pleiades cluster.
V0675 Tau |In the region of the Pleiades cluster. Not a member
V0675 Tau |of the cluster.
V0676 Tau |In the region of the Pleiades cluster.
V0677 Tau |The member of the Pleiades cluster.
V0678 Tau |In the region of the Pleiades cluster. Not a member
V0678 Tau |of the cluster.
V0679 Tau |The member of the Pleiades cluster.
V0680 Tau |In the region of the Pleiades cluster. Not a member
V0680 Tau |of the cluster.
V0681 Tau |In the region of the Pleiades cluster.
V0682 Tau |In the region of the Pleiades cluster.
V0683 Tau |In the region of the Pleiades cluster.
V0684 Tau |In the region of the Pleiades cluster. Not a member
V0684 Tau |of the cluster.
V0685 Tau |In the region of the Pleiades cluster. Not a member
V0685 Tau |of the cluster.
V0686 Tau |In the region of the Pleiades cluster.
V0687 Tau |In the region of the Pleiades cluster.
V0688 Tau |In the region of the Pleiades cluster.
V0689 Tau |In the region of the Pleiades cluster.
V0690 Tau |In the region of the Pleiades cluster.
V0691 Tau |In the region of the Pleiades cluster.
V0692 Tau |In the region of the Pleiades cluster. Possible member
V0692 Tau |of the cluster.
V0693 Tau |In the region of the Pleiades cluster.
V0694 Tau |In the region of the Pleiades cluster.
V0696 Tau |The member of the Hyades cluster.
V0697 Tau |The member of the Hyades cluster.
V0698 Tau |Type INB?
V0700 Tau |The member of the Pleiades cluster.
V0701 Tau |In the region of the Pleiades cluster.
V0702 Tau |In the region of the Pleiades cluster.
V0703 Tau |The member of the Pleiades cluster.
V0705 Tau |In the region of the Pleiades cluster.
V0706 Tau |In the region of the Pleiades cluster.
V0707 Tau |In the region of the Pleiades cluster.
V0709 Tau |In the region of the Pleiades cluster.
V0710 Tau |VB A (B 16m, 3.5", 180deg).
V0711 Tau |VB A (B 8.83m, A = 8.023", E = 0.18, Porb = 2101 yr);
V0711 Tau |SB2 (Porb = 2.83774d [10070]).
V0711 Tau |Migration period of the distortion wave is about
V0711 Tau |10.5 yr [10072].
V0711 Tau |The range of combined light variation is given.
V0712 Tau |In the region of the Pleiades cluster.
V0713 Tau |In the region of the Pleiades cluster.
V0714 Tau |In the region of the Pleiades cluster.
V0715 Tau |In the region of the Pleiades cluster.
V0716 Tau |In the region of the Pleiades cluster.
V0717 Tau |In the region of the Pleiades cluster.
V0718 Tau |In the region of the Hyades cluster.
V0725 Tau |SB1 (Porb = 110.8d [10076]).
V0725 Tau |X-ray outbursts occur periodically near
V0725 Tau |the periastron passages of the pulsar with P = Porb.
V0725 Tau |The amplitude of the corresponding variations of
V0725 Tau |visual brightness of the system A(V) = 0.03m. The period
V0725 Tau |of pulsar rotation Prot var [10077].
V0725 Tau |Prot = 104.17s (JD2442531), 103.806s (JD2442728),
V0725 Tau |103.882s (JD2443505), 103.8402s (JD2443620)
V0725 Tau |[10074]; 103.647s (JD2444521), 103.423s
V0725 Tau |(JD2445292), 103.3429ss(JD2445623) [10078].
V0726 Tau |Min II 11.2.
V0727 Tau |In the region of the Pleiades cluster.
V0728 Tau |In the region of the Pleiades cluster. Not a member
V0728 Tau |of the cluster.
V0729 Tau |Max = 2439024.46 + 152.35d*E (JD2438680 - 39415);
V0729 Tau |Max = 2440127.78 + 313.86d*E (JD2439415 - 40510).
V0729 Tau |H2O maser.
V0732 Tau |In the region of the Pleiades cluster.
V0733 Tau |In the region of the Pleiades cluster.
V0734 Tau |In the region of the Pleiades cluster.
V0735 Tau |In the region of the Pleiades cluster.
V0736 Tau |In the region of the Pleiades cluster.
V0737 Tau |In the region of the Pleiades cluster.
V0738 Tau |In the region of the Pleiades cluster. The chart in [08559]
V0738 Tau |is wrong.
V0739 Tau |In the region of the Pleiades cluster.
V0740 Tau |In the region of the Pleiades cluster.
V0741 Tau |In the region of the Pleiades cluster.
V0742 Tau |In the region of the Pleiades cluster.
V0743 Tau |In the region of the Pleiades cluster.
V0744 Tau |In the region of the Pleiades cluster.
V0746 Tau |In the region of the Pleiades cluster.
V0747 Tau |In the region of the Pleiades cluster.
V0748 Tau |In the region of the Pleiades cluster.
V0749 Tau |In the region of the Pleiades cluster.
V0750 Tau |In the region of the Pleiades cluster.
V0751 Tau |In the region of the Pleiades cluster.
V0752 Tau |In the region of the Pleiades cluster.
V0753 Tau |In the region of the Pleiades cluster. Not a member
V0753 Tau |of the cluster.
V0754 Tau |In the region of the Pleiades cluster.
V0755 Tau |In the region of the Pleiades cluster.
V0756 Tau |In the region of the Pleiades cluster.
V0757 Tau |In the region of the Pleiades cluster.
V0758 Tau |In the region of the Pleiades cluster. Not a member
V0758 Tau |of the cluster.
V0759 Tau |In the region of the Pleiades cluster.
V0760 Tau |In the region of the Pleiades cluster.
V0761 Tau |In the region of the Pleiades cluster. Not a member
V0761 Tau |of the cluster.
V0762 Tau |In the region of the Pleiades cluster. Not a member
V0762 Tau |of the cluster.
V0763 Tau |In the region of the Pleiades cluster.
V0764 Tau |In the region of the Pleiades cluster.
V0765 Tau |In the region of the Pleiades cluster.
V0767 Tau |In the region of the Pleiades cluster.
V0768 Tau |In the region of the Pleiades cluster.
V0769 Tau |In the region of the Pleiades cluster.
V0770 Tau |In the region of the Pleiades cluster.
V0771 Tau |In the region of the Pleiades cluster.
V0772 Tau |In the region of the Pleiades cluster.
V0773 Tau |There are also quasisinusoidal light variations with
V0773 Tau |P = 3.43d and A(V) = 0.13m [10056].
V0774 Tau |VB A (B 6.96m, G5IV, 66.8", 315deg).
V0775 Tau |The member of the Hyades cluster.
V0776 Tau |VB A (B 7.5m, 1.4", 333deg, 1958; C 8.7m, 77.2", 233deg,
V0776 Tau |1925); SB1 (Porb = 57.25d). The member of the
V0776 Tau |Hyades cluster.
V0777 Tau |VB A (B 8.12m V, 0.0088", 173.2deg, 1980.6).
V0777 Tau |The member of the Hyades cluster.
V0778 Tau |Min II 17.0. P var. Min I = 2438680.546 + 0.434842d*E
V0778 Tau |(JD2436528 - 38841); Min I = 2439765.488 + 0.434846d*E
V0778 Tau |(JD2439559 - 41031); since JD2440129 - see Table.
V0780 Tau |VB A (B 15.8m V, 0.3", 310deg, 1974); mu = 0.364",
V0780 Tau |P = 163deg.
V0781 Tau |Min II 9.3.
V0782 Tau |In the region of the Pleiades cluster.
V0783 Tau |In the region of the Pleiades cluster.
V0784 Tau |In the region of the Pleiades cluster.
V0785 Tau |The member of the Pleiades cluster.
V0787 Tau |In the region of the Pleiades cluster.
V0788 Tau |In the region of the Pleiades cluster.
V0789 Tau |The member of the Pleiades cluster.
V0790 Tau |The member of the Pleiades cluster.
V0791 Tau |In the region of the Pleiades cluster.
V0792 Tau |Near V752 Tau. Identical to it?
V0792 Tau |In the region of the Pleiades cluster.
V0793 Tau |The member of the Pleiades cluster.
V0794 Tau |In the region of the Pleiades cluster. Not a member
V0794 Tau |of the cluster.
V0795 Tau |In the region of the Pleiades cluster.
V0796 Tau |The member of the Pleiades cluster.
V0797 Tau |In the region of the Pleiades cluster. Not a member
V0797 Tau |of the cluster.
V0798 Tau |In the region of the Pleiades cluster.
V0799 Tau |In the region of the Pleiades cluster.
V0800 Tau |In the region of the Pleiades cluster.
V0801 Tau |In the region of the Pleiades cluster.
V0802 Tau |In the region of the Pleiades cluster.
V0804 Tau |In the region of the Pleiades cluster.
V0805 Tau |The member of the Hyades cluster.
V0807 Tau |VB A (B = GH Tau, 21.4", 193deg).
V0808 Tau |Porb = 11.93d. The member of the Hyades cluster.
V1144 Tau |SB, Porb = 13.88d.
V1148 Tau |Type LBV: is also possible. SB, Porb = 2.2075d.
V1152 Tau |Type E: with P = 11.080d is also possible.
V1161 Tau |Variability needs confirmation.
V1212 Tau |Dwarf nova in Taurus.
alf   Tau |VB A (B 13.5m, M2V, 31", 110deg).
alf   Tau |The star is surrounded by an infrared emission envelope
alf   Tau |with the diameter of about 10". In the region of the
alf   Tau |Hyades cluster.
zet   Tau |Min II 3.05.
tet 2 Tau |VB A (B 4.85m, 0.02077", 19.6deg, 1980.59); SB1 (Porb =
tet 2 Tau |140.728D, E = 0.75 [10087]). The value of P1(A1 = 0.017m B)
tet 2 Tau |is given in the Table. P1 var. Later P1 = 0.07541d
tet 2 Tau |(A1 = 0.023m B), P2 = 0.0831d (A2 = 0.013m B). Possibly
tet 2 Tau |eclipsing with the elements:
tet 2 Tau |Min = 2445358.38 + 140.734d*E, A = 0.02m B.
tet 2 Tau |The member of the Hyades cluster.
lam   Tau |Min II 3.54. Triple system. The eclipsing system rotates
lam   Tau |around the third component with P = 33.025d [10090].
lam   Tau |In the region of the Hyades cluster.
rho   Tau |The member of the Hyades cluster.
ups   Tau |VB A (B 6.5m, 0.020"). The member of the Hyades cluster.
U     Tel |P var. Before JD2421000 Max = 2420992 + 439.13d*E [00001];
U     Tel |since JD2423000 - see Table.
RR    Tel |During 1889 - 1930 12m - 14m pg (according to [00625],
RR    Tel |irregular variations; according to [00017],
RR    Tel |Max = 2411490 + 384d*E, with irregularities). During
RR    Tel |1930 - 1944 12.5m - 16.5m pg, Max = 2430145 + 386.73d*E
RR    Tel |[01649]; after 1938 an increase of mean brightness
RR    Tel |and of the amplitude was noted. An outburst from
RR    Tel |14m to 7m in October, 1944. In Max, 6.5m - 7.5m pg,
RR    Tel |during JD2431500 - 33000; after JD2433100 began
RR    Tel |to decline its mean brightness. Near the Max of the
RR    Tel |outburst no periodic variations was noted. During
RR    Tel |JD2441426 - 44899 5.06m - 6.74m J, P = 387d [09989],
RR    Tel |M - m = 0.5P; Min (V) = 2442551 + 374.2d*E (1961 - 1981),
RR    Tel |Delta(V) = 0.25m for periodic changes [10029];
RR    Tel |9.8m - 10.7m B, P = 395d (JD2443500 - 45500) [10030].
RR    Tel |In the Max of the outburst the spectrum was F5
RR    Tel |without emissions. During the brightness decline a
RR    Tel |rich emission spectrum was formed with lines of
RR    Tel |hydrogen, forbidden lines of metals in high stages
RR    Tel |of ionization, etc. Since the 1970-ies TiO absorption
RR    Tel |bands are being noted. Radio source, soft X-ray source.
RS    Tel |Semiregular variations, P = 45.8d [08140]. IR excess.
RV    Tel |VB (0.6", 294deg, 1946). d = 0.02P.
ST    Tel |The chart in [06286] is wrong.
SZ    Tel |Possibly identical with the star alpha = 18h 13m 16s,
SZ    Tel |delta = -53deg 39.2', 1950.0 (RR, 15m - 16.5m pg) [10032].
SZ    Tel |In the region of the globular cluster NGC 6584.
TT    Tel |In the region of the globular cluster NGC 6584.
TU    Tel |In the region of the globular cluster NGC 6584.
TV    Tel |In the region of the globular cluster NGC 6584.
TW    Tel |In the region of the globular cluster NGC 6584. The chart
TW    Tel |in [06286] is wrong.
TX    Tel |In the region of the globular cluster NGC 6584. The chart
TX    Tel |in [06286] is wrong.
UY    Tel |VB.
AG    Tel |nf star of a pair.
AK    Tel |Very red.
AX    Tel |[A/H] = -0.7.
BL    Tel |The depth of Min II - 0.1m pg.
BL    Tel |Semiregular variability of pulsational character
BL    Tel |(7.09m - 7.26m V) is observed outside eclipses; sometimes
BL    Tel |it may be represented by P = 65.1d, but sometimes (1969)
BL    Tel |it cannot be traced.
BO    Tel |[A/H] = -0.3.
CK    Tel |VB B (A 15.0m).
DZ    Tel |sf star of a pair.
FR    Tel |D >= 0.23P. Min II 14.0?
GH    Tel |P ~10.342d is possible.
GM    Tel |VB A.
GR    Tel |The chart in [06286] is wrong.
GY    Tel |Min II 12.0.
HH    Tel |P var slightly.
HO    Tel |Min II 8.67.
HR    Tel |EW type with twice longer P is possible.
IL    Tel |The elements need confirmation.
IQ    Tel |Min II 12.7.
KK    Tel |B - V: +0.6m: (Min light).
KN    Tel |VB A (B 16m sf).
LW    Tel |Possibly identical to NSV10695.
MT    Tel |mu alpha = -0.0127S, mu delta = -0.109".
MT    Tel |[Fe/H] = -1.82. Delta(S) = 9.9.
MV    Tel |EW type with twice longer P is possible.
MZ    Tel |EW type with twice longer P is possible.
NN    Tel |Min II 15.5.
NP    Tel |Min II 13.3.
NS    Tel |Min II 9.4.
NV    Tel |Min II 9.0.
OQ    Tel |sf star of a pair.
PR    Tel |Min II 11.35. Radio source PKS 1925 - 524.
PR    Tel |Hbeta fluctuates on ~5 min time scale.
PS    Tel |V39 (NGC 6584). Probably non-member of the cluster.
PS    Tel |P = 0.1422d or 0.1657d is possible.
PT    Tel |V27 (NGC 6584). Cluster non-member.
PU    Tel |V24 (NGC 6584). Cluster non-member.
PV    Tel |SB2.
PX    Tel |V15 (NGC 6584). Cluster non-member.
PZ    Tel |SB2.
QZ    Tel |The variability may be due to the fainter (B) component.
V0337 Tel |Type EW: is also possible.
R     Tri |P var. Max = 2412167 + 267.3d*E (JD2412000 - 16000);
R     Tri |Max = 2416972 + 262.6d*E (JD2416000 - 20000);
R     Tri |since JD2420000 - see Table. Maser (H2O).
S     Tri |P var. Max = 2418541 + 248.9d*E (JD2418000 - 31000);
S     Tri |since JD2431000 - see Table.
T     Tri |P var. Max = 2420535 + 320.6d*E (JD2420000 - 27000);
T     Tri |since JD2427000 - see Table.
U     Tri |Delta(S) = 1.3.
V     Tri |Min II 11.0.
X     Tri |VB A (B 13.3m, 6.7", 55.3deg, 1952). Usual brightness in
X     Tri |Max 8.88. d = 0.013P; Min II 9.07. According to [10043],
X     Tri |a two-peaked flare-like event of 35 min duration
X     Tri |(Delta(V) = 0.33m) was observed at JD2445594.4550.
X     Tri |P var. Min = 2422722.269 + 0.9715342d*E
X     Tri |(JD2422700 - 26600); Min = 2426946.508 + 0.9715390d*E
X     Tri |(JD2426600 - 33400); Min = 2433504.397 + 0.9715290d*E
X     Tri |(JD2433400 - 35500);
X     Tri |Min = 2435687.422 + 0.9715352d*E (JD2435500 - 39200);
X     Tri |Min = 2439375.373 + 0.9715277d*E
X     Tri |(JD2439200 - 42500) [07603]; since JD2442500 - see Table.
Y     Tri |Var No.2 (M33). VB A (B 17.28m B, 26.4" np).
RS    Tri |VB A (B 11.98m, 6.0", 214deg, 1962).
RS    Tri |d = 0.016P; Min II 10.4, Min II - Min I = 0.56P.
RU    Tri |VB A (B 12m, 21.8", 88deg). Min II 11.8:.
RW    Tri |The depth of Min I 1.12m - 2.21m.
RW    Tri |D = 0.052P - 0.086P, d ~0.03P. P var? [03434,09858,9859].
RW    Tri |Strong fluctuations of light outside eclipses. the lower
RW    Tri |the brightness outside the eclipse, the deeper the Min.
RW    Tri |In J, K light Min II of 0.16m J depth was found at the
RW    Tri |phase 0.50P [10053]. Flat spectrum of the accretion disc
RW    Tri |with emission lines.
RX    Tri |Max = 2426577 + 192d*E (JD2426500 - 31800);
RX    Tri |since JD2432800 - see Table. According to [04029],
RX    Tri |P = 100d?
RY    Tri |Red.
ST    Tri |Min II 14.5.
SW    Tri |Blazhko effect is possible.
SY    Tri |Blazhko effect is possible.
TT    Tri |In the region of the galaxy M 33.
TZ    Tri |ADS 1697 A (B 6.72m, F6V, SB2, Porb = 2.2365d,
TZ    Tri |3.9", 71deg, 1973); SB2 (P = 14.732d). Secondary
TZ    Tri |variations on ~100d time scale. H and K CaII emission was
TZ    Tri |noted only for one of the two G-stars.
alf   Tri |SB (Porb = 1.767 d).
R     TrA |SB?
U     TrA |For moments of Max0 (fundamental mode) see Table.
U     TrA |Max1 (first overtone) = 2443266.05 + 1.824881d*E.
RR    TrA |Min II 10.60, dII = 0.025P.
RW    TrA |(k - b)2 = 0.30. Delta(S) = 1.
SU    TrA |The chart in [06286] is wrong.
TW    TrA |VB.
TY    TrA |The chart in [06286] is wrong.
UW    TrA |The chart in [06286] is wrong.
UZ    TrA |The chart in [06286] is wrong.
XX    TrA |The chart in [06286] is wrong.
XY    TrA |The chart in [06286] is wrong.
AS    TrA |Min II 15.7.
BH    TrA |According to [04637], L type.
CI    TrA |Possibly P < 0.3d.
DI    TrA |The chart in [06286] is wrong.
DV    TrA |Three Max and three Min are observed during a cycle.
DV    TrA |Max1 (phi = 0.0P) 13.2m; Max2 (phi = 0.2P) 14.2m; Max3
DV    TrA |(phi = 0.6P) 13.5m. Min1, Min2, Min3 ~16.0m.
DZ    TrA |The chart in [06286] is wrong.
EH    TrA |Shallow Min II is possible.
EK    TrA |n star of a pair.
EK    TrA |For the mean cycle between normal maxima see Table. The
EK    TrA |mean cycle between supermaxima 442.1d (JD2435200 - 39700),
EK    TrA |551.5d (JD2439700 - 44050). Superhumps (delta(M) = 0.26m V)
EK    TrA |with P = 0.06492d, M - m = 0.26P [09945].
EL    TrA |Min II 10.9.
EM    TrA |Min II 10.4.
EN    TrA |According to [07934], RV: type.
EP    TrA |Min II 9.5.
EQ    TrA |Min II 9.0.
EQ    TrA |P var. Min = 2416267.614 + 2.709220d*E (JD2416000 - 29000);
EQ    TrA |since JD2429000 - see Table.
ER    TrA |P > 220d.
FH    TrA |The elements need confirmation.
FK    TrA |The elements need confirmation.
FM    TrA |P >= 220d.
GN    TrA |Min II 12.0.
HP    TrA |Deep Min II. The elements need improvement.
HV    TrA |Min II? 14.8. Min II - Min I = 0.55P.
IM    TrA |P >= 150d. Epoch of Min is given.
IW    TrA |Min II 14.5:. The elements need confirmation.
KX    TrA |2U 1639-62? P.K.326 -10deg 1. Gas velocities up to
KX    TrA |5000 km/s [09958].
KY    TrA |TrA X-1 = A1524-61.
KZ    TrA |4U 1626-67. Lx/Lopt ~2000. VB B (A 14.9m; B25", 189deg).
KZ    TrA |Barycentric period parameters for pulses [04534]: Min =
KZ    TrA |JED 2443931.2394789; P = 7.6776762s, DP/dt =
KZ    TrA |(-4.95 +-0.02)*10**(-11). Delta(m) pulse = 0.02m - 0.17m.
KZ    TrA |Porb = 2491.06s or 2492.32s [04558].
KZ    TrA |Flares with Delta(m) up to 0.4m with intervals ~20 min
KZ    TrA |correlated with X-ray flares [04536].
LM    TrA |The chart in [08661] is wrong.
LP    TrA |VB A (B 11.5m, 25", 123deg; C 12.0m, BC 6").
T     Tuc |P var. Max = 2410138 + 250.76d*E (JD2410000 - 14400);
T     Tuc |Max = 2414900 + 248.88d*E (JD2414400 - 22000);
T     Tuc |Max = 2432160 + 250.00d*E (JD2422900 - 35000);
T     Tuc |since JD2437700 - see Table.
U     Tuc |In the region of the Small Magellanic Cloud.
U     Tuc |SMS non-member.
U     Tuc |P var. Max = 2421190 + 258.12d*E (JD2412600 - 22000);
U     Tuc |Max = 2427487 + 262.83d*E (JD2422000 - 28000);
U     Tuc |Max = 2437808 + 257.70d*E (JD2428000 - 39150);
U     Tuc |since JD2440900 - see Table.
V     Tuc |In the region of the Small Magellanic Cloud.
V     Tuc |SMS non-member.
V     Tuc |The depth of Min II 0.11m.
W     Tuc |(k - b)2 = 0.09, Delta(S) = 7:. P var?
RR    Tuc |In the region of the Small Magellanic Cloud.
RR    Tuc |VB A (B 17m, 6", 90deg).
RV    Tuc |In the region of the Small Magellanic Cloud. VB.
SS    Tuc |In the region of the Small Magellanic Cloud. HV 1877.
SS    Tuc |Earlier was erroneously identifded with HV 1887.
SU    Tuc |In the region of the Small Magellanic Cloud. HV 1922.
SU    Tuc |According to [09980], alternatively may be identical to
SU    Tuc |HV 1920.
SX    Tuc |In the region of the Small Magellanic Cloud. VB (B 16m? P).
SY    Tuc |In the region of the Small Magellanic Cloud. Min II 15.4.
TV    Tuc |In the region of the Small Magellanic Cloud.
TV    Tuc |The variable's position in 2' to the north
TV    Tuc |of CPD -73deg 64 [09980] makes it impossible to identify
TV    Tuc |it with HV 2041.
TZ    Tuc |In the region of the Small Magellanic Cloud.
TZ    Tuc |SMS non-member.
TZ    Tuc |VB A (B 13m sp).
UW    Tuc |In the region of the Small Magellanic Cloud.
UW    Tuc |SMC non-member.
UX    Tuc |In the region of the Small Magellanic Cloud.
UX    Tuc |SMS non-member.In the neighbourhood OF 47 Tuc; probably
UX    Tuc |cluster non-member. P var. [Fe/H] = -1.8.
YY    Tuc |The elements need improvement; current elements with the
YY    Tuc |epoch from [07984] are given.
YY    Tuc |(k - b)2 = 0.03. Delta(S) = 8:.
AD    Tuc |In the region of the Small Magellanic Cloud.
AD    Tuc |SMS non-member. Delta(S) = 4.9.
AF    Tuc |In the region of the Small Magellanic Cloud. SMS
AF    Tuc |non-member.
AH    Tuc |In the region of the Small Magellanic Cloud. SMS
AH    Tuc |non-member. P var.
AI    Tuc |In the region of the Small Magellanic Cloud. SMS
AI    Tuc |non-member. In the region of the globular cluster NGC 362.
AI    Tuc |P var.
AK    Tuc |In the region of the Small Magellanic Cloud. SMS
AK    Tuc |non-member. P var.
AL    Tuc |In the region of the Small Magellanic Cloud. SMS
AL    Tuc |non-member.
AM    Tuc |The elements should be checked.
AM    Tuc |[Fe/H] = -1.82. Delta(S) = 9.9.
AO    Tuc |The elements need improvement. Delta(S) = 5.
AP    Tuc |In the region of the Small Magellanic Cloud. SMS
AP    Tuc |non-member.
AQ    Tuc |In the region of the Small Magellanic Cloud. SMS
AQ    Tuc |non-member.In the region of the globular cluster 47 Tuc.
AQ    Tuc |Min II 10.48.
AR    Tuc |In the region of the Small Magellanic Cloud. SMS
AR    Tuc |non-member.
AU    Tuc |In the region of the Small Magellanic Cloud. SMS
AU    Tuc |non-member.
AV    Tuc |In the region of the Small Magellanic Cloud. SMS
AV    Tuc |non-member.
BD    Tuc |In the region of the Small Magellanic Cloud. SMS
BD    Tuc |non-member.
BE    Tuc |In the region of the Small Magellanic Cloud.
BF    Tuc |In the region of the Small Magellanic Cloud. [A/H] = -0.7.
BG    Tuc |In the region of the Small Magellanic Cloud. SMS
BG    Tuc |non-member.
BH    Tuc |In the region of the Small Magellanic Cloud. VB A
BH    Tuc |(B 14.28m, 10" n).
BS    Tuc |(k - b)2 = 0.10.
BZ    Tuc |P var. Max = 2429849.448 + 127.78d*E (JD2410000 -
BZ    Tuc |35100) [03641]; Max = 2441193.541 +127.27d*E
BZ    Tuc |(JD2435100 - 43500) [A.M. van Genderen, AsAp Suppl 52,
BZ    Tuc |423, 1983]; since JD 2443500 - see Table.
CF    Tuc |In the region of the Small Magellanic Cloud. SMS
CF    Tuc |non-member. Soft X-ray source. Distortion
CF    Tuc |wave. Delta(m) = 0.057m [10065]. Min II 7.52.
DX    Tuc |Type RRC: is also possible.
tet   Tuc |For the period of the main oscillation (A = 0.0132m) see
tet   Tuc |Table. Other instable frequences were also noted.
R     UMa |Maser (H2O).
S     UMa |S 1.5/6 e. P var. Max = 2398325 + 224.51d*E
S     UMa |(JD2394000 - 2405000); Max = 2405290 + 230.20d*E
S     UMa |(JD2405000 - 10500); Max = 2417530 + 223.96d*E
S     UMa |(JD2410500 - 23500); Max = 2426324 + 228.53d*E
S     UMa |(JD2423500 - 28800); since JD2428800 - see Table.
T     UMa |Maser (H2O).
W     UMa |ADS 7494 A (B 12.35m, 6.5", 44deg, 1963).
W     UMa |dI = 0.037P; Min II 8.43, dII = 0.028P.
W     UMa |Soft X-ray source. LX/Lbol = 1.7*10**(-4).
W     UMa |P var. Min I = 2420980.8093 + 0.333638880d*E
W     UMa |(JD2416000 - 21000); Min I = 2420980.8093 +
W     UMa |0.333636993d*E (JD2421000 - 33000) [01760];
W     UMa |Min I = 2435918.4169 + 0.33363832d*E (JD2433000 - 41000)
W     UMa |[05327]; since JD2441000 - see Table. The light curve shape,
W     UMa |including depths of minima, var. A moving wave with
W     UMa |Delta(m) = 0.025m y and P ~1100d [10067] was noted. A
W     UMa |flare (Delta(m) = 1.5m, lambda 3300 A,
W     UMa |delta(lambda) = 50 A, JD2438511.7,
W     UMa |delta(t) = 7 min) was announced [05788]. The system
W     UMa |contains gaseous streams, dark spots on the surface of
W     UMa |the components. H and K CaII emission.
Z     UMa |Usually 2 Max and 2 Min during a cycle.
RV    UMa |P var. Max = 2417861.434 + 0.4680618d*E
RV    UMa |(JD2417800 - 25000); Max = 2425053.675 + 0.4680654d*E
RV    UMa |(JD2425000 - 29000) [00188];
RV    UMa |Max = 2438459.945 + 0.468062d*E (JD2429000 - 40000) [03506];
RV    UMa |since JD2440000 - see Table. Blazhko effect, Pi = 92.12d
RV    UMa |(JD2436229 - 38114) [09835]. Pi var. [Fe/H] = -1.04;
RV    UMa |Delta(S) = 3.5.
RW    UMa |DI < 0.08P; Min II 10.34, DII = 0.10P.
RW    UMa |[Fe/H]A = -0.1, [Fe/H]B = -1.0. P var?
RW    UMa |Distortion wave, A = 0.11m V.
SU    UMa |The cycle of normal maxima 5d - 35d [09782,03791].
SU    UMa |Three different mean values of the mean cycle of
SU    UMa |supermaxima change each other being active at different
SU    UMa |time intervals: P1 = 161.5d; P2 = 203.9d; P3 = 248.1d
SU    UMa |(<P> = 201.7d) [09276]. Porb = 2.06d/N (N = 26, 27, 28)
SU    UMa |or 3.1h. Surrounded by a faint halo (28' diameter) of soft
SU    UMa |X-ray sources.
SW    UMa |SB. Superior conjunction of the accretion disc
SW    UMa |T = 2445376.8601 + 0.0567433d*E [09836].
SX    UMa |P var strongly. Before JD2418800
SX    UMa |Max = 2416200.486 + 0.3071148d*E;
SX    UMa |Max = 2418800.213 + 0.3071345d:*E (JD2418800 - 22500)
SX    UMa |[00001]; Max = 2422653.5032 + 0.30711855d*E
SX    UMa |(JD2422500 - 26000) [10083]; Max = 2426400.418 +
SX    UMa |0.3071555d*E (JD2426000 - 29500); Max =
SX    UMa |2430000.250 + 0.3071301d*E (JD2429500 - 34000),
SX    UMa |Max = 2438508.751 + 0.3071363d*E (JD2434000 - 39000);
SX    UMa |since JD2441500 - see Table. [Fe/H] = -1.82,
SX    UMa |Delta(S) = 9.9.
SZ    UMa |mu alpha = -0.4853s, mu delta = +0.148".
TU    UMa |P var [03506]. [Fe/H] = -1.05, Delta(S) = 7.6.
TW    UMa |d = 0.002P; Min II 12.3:.
TX    UMa |Min II 7.13. P var. Min I = 2416426.801 + 3.063297d*E
TX    UMa |(JD2416000 - 22000); Min I = 2427926.492 + 3.063337d*E
TX    UMa |(JD2424200 - 30000); Min I = 2433440.431 + 3.063300d*E
TX    UMa |(JD2430000 - 38000) [09839]; since JD2438000 - see Table.
TY    UMa |P var, non-linear term: +6.4d*10**(-11)*E**2.
TY    UMa |dI = 0.05P, dII = 0.00P. The light curve shape var.
TY    UMa |12.10 <= Min I <= 12.14, 12.06 <= Min II <= 12.12.
UX    UMa |The shape of the eclipse light curve, the
UX    UMa |mean level of light outside eclipses, the depth of
UX    UMa |Min var. Deviations from the tabulated elements may
UX    UMa |reach  +-0.002d. Rapid brightness oscillations
UX    UMa |(28.54s <= P <= 30.02s) are sometimes observed [07304].
UX    UMa |Soft X-ray source.
UY    UMa |Min II 12.9.
VV    UMa |Min II 10.26. P var. Min I = 2439245.408 + 0.6873793d*E
VV    UMa |(JD2425600 - 40200) [09843]; Min I = 2440768.6280 +
VV    UMa |0.687367d*E (JD2440200 - 42700); since JD2442700 - see
VV    UMa |Table.
VX    UMa |Maser (H2O).
WX    UMa |Mu alpha = -0.4094s, mu delta = +0.955", VB B
WX    UMa |(A = BD +44deg 2051, dM2, 8.74m V; B 28", 133deg;
WX    UMa |common mu). Soft X-ray source. LX/LV = 0.095.
XY    UMa |Mu alpha = -0.0055s, mu delta = -0.175". P var.
XY    UMa |Non-linear term:  +2.77d*10**(-11)*E**2.
XY    UMa |The brightness outside eclipses var by 0.16m V. The depth
XY    UMa |of Min I is 0.48m - 0.67m, that of Min II is 0.19m.
XY    UMa |Migrating wave.
XZ    UMa |Min II 10.2. P var? Min = 2444986.445 + 1.2223105d*E
XZ    UMa |(JD2414990 - 45000); since JD2445000 - see Table.
AA    UMa |Min II 11.53, Max II 10.94. The elements should
AA    UMa |be checked.
AC    UMa |VB B (A = BD  + 65G671, 9.97m V, B-V = +0.50m; B 19",
AC    UMa |114deg, 1957). The chart in [08953] is wrong.
AD    UMa |Blazhko effect is possible. Pi = 35d - 40d,
AD    UMa |delta(A) = 0.2m.
AE    UMa |The fundamental mode P0 is given in the Table.
AE    UMa |P1 = 0.066527d, Pbeat = 0.293616d [09869].
AE    UMa |Max 10.86 - 11.10, Min 11.46 - 11.52.
AF    UMa |d = 0.05P.
AK    UMa |The elements need improvement.
AN    UMa |The epoch of Min for periodic (P = Porb) light variations
AN    UMa |with A <= 1m B is given. Min II is present. B - V = 0.0
AN    UMa |in Max light,  +0.5 during an eclipse; U - B = -1.1.
AN    UMa |Circular polarization in B light -9% to -35%; linear
AN    UMa |polarization 0% - 13% with a sharp Max near Max light.
AN    UMa |Rapid changes (A = 0.03m, f = 0.4 - 0.8 Hz). The mean
AN    UMa |light level and the light curve shape var. During the low
AN    UMa |state (B ~19m) the light variability with porb disappears,
AN    UMa |emission lines occur only during 10% of Porb, IR excess is
AN    UMa |noted. Soft X-ray source, var. Emissions of H, HeI,
AN    UMa |He II, NIII, FeII.
AW    UMa |dI = 0.06P:; Min II 7.08, dII = 0.11P.
AW    UMa |The light curve shape var.
AW    UMa |P var. Min I = 2442150.4385 + 0.43873234d*E
AW    UMa |(JD2438000 - 42200); since JD2442200 - see Table.
AX    UMa |P var. Max = 2435951.354 + 0.53510d*E (JD2435900 - 38200)
AX    UMa |[04375]; during JD2445000 - 45900 - see Table.
BE    UMa |d = 0.006P. Outside eclipses var
BE    UMa |14.8m <= B <= 16.0m (reflection effect). The depth of
BE    UMa |eclipses for lambda lambda 3330 - 3700 A is greater than
BE    UMa |4.3m,that for lambda lambda 5265 - 6005 A is 1.5m.
BG    UMa |Min II 10.93. Alternative type EW.
BH    UMa |Min II 12.3.
BI    UMa |Min II 15.8.
BK    UMa |[Fe/H] = -1.29, Delta(S) = 6.6.
BL    UMa |Min II 16.2.
BM    UMa |The depth of Min II 0.80m.
BN    UMa |[Fe/H] = -1.65, Delta(S) = 8.9.
BP    UMa |D <= 0.04P. The elements need confirmation.
CE    UMa |In the region of the cluster of galaxies Abell 1213.
CE    UMa |SN 1966 omicron?
CF    UMa |Groombridge 1830 B (A = BD +38deg 2285, V = 6.45m,
CF    UMa |B - V = +0.75m, G8 subdwarf, mu alpha =  + 0.339s,
CF    UMa |mu delta = -5.81"; B 2", 165deg). A possible flare on
CF    UMa |February 27, 1968. A brightening of the combined light by
CF    UMa |0.6m pg on April 27, 1939 [09881]. Maybe the object does
CF    UMa |not exist [09882].
CH    UMa |X-ray source 1E 1003 +67. LX/Lopt = 0.04.
CM    UMa |P var?
CQ    UMa |The epoch of Max in U and B light
CQ    UMa |coinciding with that of Min in V light is given.
CQ    UMa |A(U) = 0.06m, A(B) = 0.06m.
CR    UMa |The elements for Max in U light are given. In B and V
CR    UMa |bands no periodicity is apparent. A(U) = 0.03m.
CW    UMa |Mu = 0.27", P = 300deg.
DF    UMa |ADS 8242A (B 11.4m, 1.8", 60deg, 1960).
DF    UMa |The data for combined brightness are given in the Table.
DF    UMa |SB1, Porb = 1.033824d. Mu alpha =  +0.0131s,
DF    UMa |mu delta = -0.038". Besides rapid variations (<V> = 10.14m,
DF    UMa |Delta(V) = 0.05m), long term variations are possible.
DG    UMa |Blazhko effect is possible.
DK    UMa |Soft X-ray source, lg Lx/Lv = -3.5. [Fe/H] = -0.38.
DL    UMa |Eclipses with P = 0.42d [04706].
DM    UMa |SB1 (Porb = 7.492d).
DM    UMa |Min = 2444026.97 + 7.478d*E (1979 - 1982);
DM    UMa |1981 - 1984 - see Table. Two Min in the light curve in
DM    UMa |1981 - 1982.
DN    UMa |ADS 8347 ABC (A 7.2m vis; B 9.0m vis, 0.121", 142.0deg,
DN    UMa |1981.5; C 8.3m vis, 4.0", 42deg, 1980; D = BS 4561,
DN    UMa |A1pCrEuSr:, V = 7.03m, B - V = +0.01m, 63.0", 114deg).
DN    UMa |The range of combined brightness for the three components
DN    UMa |is given. It is not known which of the components varies.
DN    UMa |The component D was used as a comparison star.
DN    UMa |Min II 6.73, Min II - Min I = 0.504P.
GM    UMa |SB, discrepant Porb = 3.2424d.
HH    UMa |Type EW: is also possible.
HN    UMa |Type DSCT: is also possible.
HU    UMa |VB A (B = GSC 3014.0222 = L265-581, 24", 250 deg, common proper
HU    UMa |motion).
II    UMa |Type RR: is also possible.
eps   UMa |SB (P=4.15A). Interferometric binary? (0.053", 94.5deg,
eps   UMa |1975.4). In 1976 - 1983 attempts to resolve the binary
eps   UMa |interferometrically were not successful.
eps   UMa |In the UMa moving cluster; mu alpha = +0.0131s,
eps   UMa |mu delta = -0.010".
ups   UMa |ADS 7534 A (B 11.5m, 11.3", 295deg, common mu).
ups   UMa |mu alpha = -0.0382s, mu delta = -0.156". The light curve
ups   UMa |shape and A var.
R     UMi |H2O maser.
S     UMi |P var. Max = 2422604 + 321.9d*E (JD2413000 - 23000);
S     UMi |Max = 2432200 + 331.5d*E (JD2423000 - 32800);
S     UMi |Max = 2436080 + 322.5d*E (JD2433000 - 37000);
S     UMi |Max = 2439011 + 326.5d*E (JD2437000 - 41500);
S     UMi |since JD2441500 - see Table.
T     UMi |P var. Max = 2428332 + 315.48d*E (JD2416500 - 29500);
T     UMi |Max = 2436415 + 310.05d*E (JD2429500 - 37200);
T     UMi |Max = 2442389 + 315.5d*E (JD2437200 - 43600); since
T     UMi |JD2443600 - see Table.
U     UMi |P var. Max = 2416975 + 323.1d*E (JD2416500 - 21000);
U     UMi |Max = 2428804 + 331.3d*E (JD2421000 - 29780) [00001];
U     UMi |Max = 2429789 + 320.6d*E (JD2429780 - 34600) [00960];
U     UMi |Max = 2434600 + 331d*E (JD2434600 - 36300);
U     UMi |Max = 2437853 + 322.6d*E (JD2436300 - 39000); since
U     UMi |JD2439000 - see Table.
V     UMi |Mean brightness var with P2 = 760d.
W     UMi |Min II 8.66; d = 0.02P. P var? Non-linear term in the
W     UMi |elements is possible: -7.7d*10**(-10)*E**2.
X     UMi |P var? Max = 2424224 + 343d*E (JD2423800 - 25100)
X     UMi |[00684]; since JD2438100 - see Table.
RR    UMi |SB (Porb = 749.4d [09896]).
RT    UMi |Min II 10.86.
RU    UMi |Min II 10.20.
RZ    UMi |Min II 13.5.
SZ    UMi |Variability needs confirmation.
alf   UMi |VB A (B 8.20m, F3V, 18.3", 218deg); SB1 (Porb = 10969d,
alf   UMi |E = 0.655 [09904]). P var. There is a non-linear term in
alf   UMi |the elements: +1.9877d*10**(-7)*E**2. The amplitude of
alf   UMi |light and radial velocity variation decreased in 1982.
alf   UMi |A(V) = 0.04m (1984).
gam   UMi |P var. Max = 2424301.78 + 0.14335d*E [10097]; Max =
gam   UMi |2427904.468 + 0.14335d*E [10098]. Elements given in the
gam   UMi |Table represent observations in 1964 - 1968. According to
gam   UMi |[09906] Vr var in 1922 with P = 0.108449d.
eps   UMi |VB A (B 12.5m, 76.9", 3deg). Min II 4.21.
S     Vel |Min II 7.83; d = 0.041P. P var? There is a non-linear term
S     Vel |in the elements given in the Table: +4.47d*10**(-9)*E**2.
W     Vel |P var. Max = 2415053 + 384.3d*E (JD2414600 - 17400);
W     Vel |Max = 2426080 + 399.9d*E (JD2422400 - 27300);
W     Vel |Max = 2429990 + 388.0d*E (JD2427300 - 30100);
W     Vel |Max = 2438328 + 398.7d*E (JD2430100 - 38800);
W     Vel |since JD2438800 - see Table. OH emission.
Y     Vel |P var. Max = 2415900 + 438.6d*E (JD2411500 - 15900);
Y     Vel |Max = 2419930 + 447.7d*E (JD2415900 - 19930);
Y     Vel |Max = 2425755 + 452.8d*E (JD2421600 - 27600);
Y     Vel |Max = 2434150 + 439.5d*E (JD2427600 - 34200);
Y     Vel |since JD2434200 - see Table.
Z     Vel |P var. Max = 2415445 + 435.96d*E (JD2415000 - 25100);
Z     Vel |Max = 2425462 + 417.99d*E (JD2425100 - 29700) [00960];
Z     Vel |since JD2429200 - see Table.
RR    Vel |Min II 10.9.
RS    Vel |P var. Max = 2410403 + 421d*E (JD2410400 - 16800)
RS    Vel |[09961]; since JD2415450 - see Table.
RU    Vel |VB A (B 12m sf). According to [00017],
RU    Vel |Max = 2414390 + 63d*E.
RW    Vel |P var. Max = 2413553 + 430.4d*E (JD2413500 - 18500);
RW    Vel |Max = 2420610 + 465.7d*E (JD2418500 - 25700); since
RW    Vel |JD2425700 - see Table.
RX    Vel |Min II 10.5.
RY    Vel |[A/H] = -0.3. P var. Max = 2440246.67 + 28.1270d*E
RY    Vel |(JD2419000 - 40250) [05366]; since JD2443900 - see Table.
SW    Vel |P var. Max = 2434872.95 + 23.473d*E - 3.75d*10**(-5)*E**2
SW    Vel |(JD2412500 - 35500) [09636]. Since JD2440700 - see Table.
SX    Vel |The light curve has double maximum. The epoch of
SX    Vel |the primary (second) maximum is given in the Table.
TT    Vel |Min II 10.7.
UW    Vel |In the region of the open cluster NGC 3033.
YZ    Vel |Min II 12.8; DII = 0.040P; Min II - Min I = 0.537P.
ZZ    Vel |Min II 10.0.
AA    Vel |Min II 9.9.
AC    Vel |Min II 9.11.
AF    Vel |(k - b)2 = 0.06. Blazhko effect is possible [10110].
AH    Vel |SB? [10111]. In the region of the open cluster
AH    Vel |Collinder 173.
AI    Vel |Mu = 0.11", P = 76deg; (k - b)2 = 0.23.
AI    Vel |Light oscillations with the period P0 given in the Table
AI    Vel |are superimposed by oscillations with P1 = 0.08620868d and
AI    Vel |twice smaller amplitude. According to [10112] P0 is
AI    Vel |constant, P1 is increasing.
AK    Vel |In the region of the open cluster Collinder 173.
AL    Vel |d = 0.072P.
AO    Vel |In the region of the open cluster Collinder 173.
AO    Vel |Min II 9.55:. There is apsidal line motion.
AO    Vel |There is a sinusoidal term in the elements given in the
AO    Vel |Table: +0.058d*sin(phi), where phi = 2pi(E - 5338)/11500,
AO    Vel |and E values are counted from JD2415810.66.
AO    Vel |Min II = 2424270.125 + 1.5845993d (E - 5338) -
AO    Vel |-0.058d*sin(phi); Min II - Min I = 0.792d - 0.116d*sin(phi).
AP    Vel |P1 = 2.19984d; P1/P0 = 0.703. M - m var (0.25P <= M - m <=
AP    Vel |<= 0.50P) [03710].
AQ    Vel |d = 0.05P. The depth of Min II 0.05m.
AS    Vel |Min II 8.4; Min II - Min I = 0.55P.
AT    Vel |d = 0.03P. In the region of the open cluster Collinder 173.
AU    Vel |In the region of the open cluster Collinder 173.
AV    Vel |In the region of the open cluster Collinder 173.
AW    Vel |In the region of the open cluster Collinder 173.
AX    Vel |The first overtone mode light variation elements with the
AX    Vel |period P1 are given in the Table; the amplitude of
AX    Vel |the first overtone mode light variation A1 exceeds
AX    Vel |that of the fundamental mode, A0:A1(V) = 1.5A0(V).
AX    Vel |For the fundamental mode P0 Max hel = 2443878.885 +
AX    Vel |3.673174d*E.
AX    Vel |P1/P0 = 0.706; M - m var: 0.24P <= M - m <= 0.50P:.
AY    Vel |Min II 9.7.
AZ    Vel |Min II 13.0. In the region of the open cluster
AZ    Vel |Collinder 173.
BB    Vel |P < 20d. In the region of the open cluster Collinder 173.
BC    Vel |Min II 12.3.
BD    Vel |d = 0.04P.
BE    Vel |Min II 12.5.
BF    Vel |The depth of Min II 0.04m.
BM    Vel |Min II 13.0. In the region of the open cluster NGC 2547.
BM    Vel |In the region of the open cluster Collinder 173.
BO    Vel |Min II 14.2.
BP    Vel |Min II 13.7.
BR    Vel |The shape of the light curve varies.
BT    Vel |Min II 14.8.
BU    Vel |Min II 10.96; Min II - Min I = 0.522P. In the region
BU    Vel |of the open cluster Collinder 173.
BV    Vel |In the region of the open cluster Collinder 173.
BW    Vel |Min II 14.3.
BX    Vel |In the region of the open cluster Tr 10.
BZ    Vel |Min II 10.4; Min II - Min I = 0.57P.
CK    Vel |D ~0.3d.
CL    Vel |Min II 13.4.
CR    Vel |d = 0.05P.
CS    Vel |[A/H] = 0.1. Possible member of the open
CS    Vel |cluster Ruprecht 79.
CU    Vel |The period of superhumps ~0.08d, A = 0.4m [10115].
CV    Vel |Min II 7.17.
CW    Vel |d = 0.024P. The depth of Min II 0.1m pg.
CZ    Vel |Min II 11.1.
DF    Vel |Min II 13.4.
DH    Vel |Min II 13.7.
DK    Vel |VB A (B 12.50m, 22", 315deg; C 16m, 10", 60deg).
DL    Vel |Min II 12.1.
DM    Vel |P = 123d?
DQ    Vel |Min II 11.0.
DS    Vel |Min II 10.8.
DT    Vel |(k - b)2 = 0.24.
DX    Vel |Min II 10.3. In the region of the open cluster Col 213.
EH    Vel |Min II 13.4.
EL    Vel |In the region of the open cluster Collinder 173.
EO    Vel |Min II 11.90, DII = 0.07P.
EO    Vel |Apsidal motion: Min II - Min I = 3.15d + 0.00003d*E.
EO    Vel |Min II = 2441716.75 + 5.32969d*E.
EP    Vel |In the region of the open cluster IC 2395.
ES    Vel |Min II 12.7.
ET    Vel |Min II 12.1.
EU    Vel |Min II 13.8.
EY    Vel |d = 0.04P:.
FM    Vel |Min II 12.9.
FS    Vel |Delta(S) = 10.
FT    Vel |Min II 10.5.
FW    Vel |Min II 10.0.
FX    Vel |Min II 10.5. The shape of the light curve varies.
FY    Vel |Min II 7.03. Type ELL? [06827].
FZ    Vel |VB A (B 12.08m, 24.2", 338deg).
GG    Vel |VB A (B 11.2m, 6", delta(alpha) = 0). P = 2.950432d?
GP    Vel |<Min II> 6.90. Min II - Min I = 0.55P.
GP    Vel |The shape of the light curve varies.
GP    Vel |There are probably long-period light
GP    Vel |oscillations: Min = 2442681.6 + 93.3d*E (A ~0.02m)
GP    Vel |[10051]. The period of X-ray pulses var: 282.8913s
GP    Vel |(1975.5) [10125]; 282.919s (1975.7) [10126]; 282.869s
GP    Vel |(1976.4), 282.838s (1976.9) [10127]; 282.80s (1978.9)
GP    Vel |[10128]; 282.745s (1979.3), 282.7874s (1980.3), 282.87s
GP    Vel |(1981.0) [10129]; 282.93s (1981.9 - 1982.9); 282.9306s
GP    Vel |(1983.2) [10078].
GV    Vel |In the region of the open cluster NGC 2660.
HU    Vel |Pulsar PSR 0833-45. In the nebula Vela SNR.
HU    Vel |Star M [08276]. The pulsed radiation varies in radio,
HU    Vel |optical and gamma rays with P = 0.089s.
HU    Vel |P var [10136 - 10139]: P = 0.089233318274s
HU    Vel |(JD2442553 - 680), P = 0.089234713929s (JD2442700 - 848),
HU    Vel |P = 0.089244007685s (JD2443654 - 676), P = 0.089245406487s
HU    Vel |(JD2443719 - 850) [10137]; P = 0.089256985348s
HU    Vel |(JD2444795.84) [10138].
HV    Vel |A member of the open cluster IC 2391.
HW    Vel |P = 0.26133d? A member of the open cluster IC 2391.
HX    Vel |VB A (B 7.1m, 0.3", 313deg, 1949); in the region
HX    Vel |of the open cluster IC 2395. Min II 5.50:.
HY    Vel |VB A (B 5.7m, 76.6"); a member of the open cluster IC 2391.
HY    Vel |Min II 4.90.
IL    Vel |A var (0.02m <= A <= 0.15m). Beat period 10.075d
IL    Vel |(Min A = 2443175.5 + 10.075d*E).
IM    Vel |VB A (B 9.73m, 3.3", 179deg, 1948).
IM    Vel |The double wave of light variations
IM    Vel |with rotation period Prot = 2.85204d and A = 0.03m is
IM    Vel |superimposed by oscillations with the periods
IM    Vel |P1 = 0.00812815d (A1 = 0.0043m), P2 = 0.00808206d
IM    Vel |(A2 = 0.0035m), P3 = 0.00810503d (A3 = 0.0008m), P4 =
IM    Vel |0.004052519d (A4 = 0.0009m), P5 = 0.004064065d
IM    Vel |(A5 = 0.0004m), P6 = 0.004041031d (A6 = 0.0004m),
IM    Vel |P7 = 0.00815128d (A7 = 0.0004m) [09208].
IN    Vel |P = 65 - 70d,
IP    Vel |VB A (B 11.2m V, 2.1", 200deg, 1929). P > 1.25d.
IQ    Vel |Min II 12.94; Min II - Min I = 0.500P.
IS    Vel |A(U) var: 0.005m <= A(U) <= 0.018m.
IT    Vel |Min II 7.08. P = 23.52d?
OQ    Vel |The type is doubtful.
V0360 Vel |Several close companions.
gam 2 Vel |VB A (B 4.22m, 41.3", 220deg).
gam 2 Vel |SB2 (Porb = 78.5002d [10119]). In HII region.
gam 2 Vel |T0 = 2433633.0 is the epoch of the conjunction where the
gam 2 Vel |O component is in front [10119].
lam   Vel |VB A (B 14.8m, 18.2", 137deg).
omi   Vel |A member of the open cluster IC 2391. P(VR) = 2.74d.
omi   Vel |P = 2.76d? SB1? The epoch of the light maximum is given.
omi   Vel |Close binary system?
R     Vir |P var. Max = 2381914 + 145.77d*E (JD2338900 - 2402000);
R     Vir |Max = 2402321 + 144.90d*E (JD2402000 - 18000);
R     Vir |Max = 2418268 + 145.48d*E (JD2418000 - 30000);
R     Vir |Max = 2430489 + 148.32d*E (JD2430000 - 34000);
R     Vir |Max = 2434193 + 144.63d*E (JD2434000 - 38500);
R     Vir |Max = 2438829 + 147.45d*E (JD2438500 - 43000);
R     Vir |since JD2443000 see Table. Maser (SiO).
S     Vir |P var. Max = 2399014 + 374.7d*E (JD2398600 - 2405000);
S     Vir |Max = 2412970 + 376.2d*E (JD2412000 - 23500, on average);
S     Vir |Max = 2423502 + 381.52d*E (JD2423500 - 23000); since
S     Vir |JD2433000 - see Table. Maser (H2O, SiO).
T     Vir |Maser (OH, H2O, SiO).
V     Vir |P var. Before JD2427000 Max = 2400467 + 250.17d*E;
V     Vir |Max = 2427225 + 246.54d*E (JD2427000 - 31500);
V     Vir |since JD2431500 - see Table.
W     Vir |The epoch of Min is given. P var.
W     Vir |Min = 2404151.168 + 17.2707d*E (JD2403000 - 23200);
W     Vir |Min = 2423200.837 + 17.2634d*E (JD2423200 - 29700);
W     Vir |since JD2429700 - see Table. The light curve shape var.
W     Vir |[Fe/H] = -1.03.
X     Vir |VB A (B 12m, dK4, 0.6', ~50deg). The brightenings
X     Vir |of 1871 and 1882 may be due to misidentification [01651].
Z     Vir |mu alpha = +0.0098S, mu delta = -0.120".
Z     Vir |P var. Max = 2409683 + 309.19d*E (JD2408000 - 18500);
Z     Vir |since JD2418500 - see Table.
RS    Vir |Maser (OH, H2O, SiO). P var. Max =2412592 + 351.29d*E
RS    Vir |(JD2412000 - 31000); since JD2431000 - see Table.
RT    Vir |Maser (OH, H2O, SiO). According to [10145], observations
RT    Vir |of 1970-1977 are not in agreement with the P value in the
RT    Vir |Table.
RU    Vir |P var? Max = 2425120 + 435.9d*E (JD2414000 - 31500); since
RU    Vir |JD2431500 - see Table.
RV    Vir |P var. Max = 2412272 + 268.39d*E (JD2412000 - 31500);
RV    Vir |since JD2431500 - see Table.
RX    Vir |VB (B 13.0m vis, 1.1", 107deg, 1939). According to
RX    Vir |photoelectric observations [06450,08837], 8.72m - 8.81m V.
RX    Vir |Const? [06450].
SS    Vir |P var. Max = 2415910 + 352.75d*E (JD2415900 - 21500);
SS    Vir |Max = 2421913 + 361.7d*E (JD2421500 - 26500);
SS    Vir |Max = 2428359 + 350.12d*E (JD2426500 - 40000);
SS    Vir |since JD2440000 - see Table.
ST    Vir |P var. Max = 2425005533 + 0.4108494d*E (JD2422000 - 29100)
ST    Vir |[10146]; Max = 2436702.513 + 0.4108168d*E
ST    Vir |(JD2433000 - 39000) [03415]; since JD2439000 - see Table.
ST    Vir |Blazhko effect? Delta(S) = 0.8.
SU    Vir |P var. Max = 2415040 + 213.7d*E (JD2415000 - 19500);
SU    Vir |Max = 2419926 + 210.96d*E (JD2415000 - 31500);
SU    Vir |Max = 2437378 + 210.2d*E (JD2431500 - 38500);
SU    Vir |since JD2438500 - see Table.
SV    Vir |P var? The mean elements are given. Maser (H2O).
SZ    Vir |Possibly EW with a very small A.
TV    Vir |VB A (B P).
TW    Vir |Porb = 0.182666d [09430]. Variability of ellipsoidal
TW    Vir |character in H light: P = Porb/2, A(H) = 0.13m.
TW    Vir |X-ray source.
TX    Vir |VB A (B 15m, 0.3' P).
TY    Vir |[Fe/H] = -1.7.
TZ    Vir |P2 = 6900d is superimposed?
UU    Vir |[Fe/H] = -0.3. delta[S] = 0.7.
UW    Vir |d = 0.011P. P var. Min = 2419942.513 + 1.8106818d*E
UW    Vir |(JD2415000 - 34500); since JD2441000 - see Table
UY    Vir |d = 0.014P; Min II 8.1.
VV    Vir |Min II 12.2:.
VW    Vir |SN 1895 (NGC 4424).
XX    Vir |[Fe/H] = -1.5. Delta(S) = 9:.
YZ    Vir |[A/H] = -0.9.
AD    Vir |P var. Max = 2425259.259 + 0.5522109d*E
AD    Vir |(JD2419000 - 31000); since JD2431000 - see Table.
AF    Vir |P var. Max = 2429051.697 + 0.4838214d*E
AF    Vir |(JD2419500 - 36000); Max = 2436718.3758 +
AF    Vir |0.4838386d*E (JD2436000 - 37500) [10159];
AF    Vir |since JD2440000 - see Table. DM var.
AG    Vir |The depth of Min II up to 0.44m.
AG    Vir |The light curve shape and A var.
AG    Vir |dI = 0.03P:, dII = 0.66P. Min II - Min I = 0.512P.
AG    Vir |P var. Min = 2434487.4297 + 0.6426489d*E
AG    Vir |(JD2424500 - 34500); since JD2434500 - see Table.
AH    Vir |mu alpha = +0.0015S, mu delta = -0.111"
AH    Vir |ADS 8472 A (B 13.2m, 1.3", 17deg).
AH    Vir |The combined brightness is given,
AH    Vir |dI = 0.07P. The depth of Min II 0.53m, dII = 0.00P.
AH    Vir |The light curve shape var.
AH    Vir |P var. Min = 2434841.3963 + 0.40751843d*E
AH    Vir |(JD2425000 - 35000) [05222]; Min = 2435573.710 +
AH    Vir |0.40752192d*E (JD2435000 - 41400); Min =
AH    Vir |2441411.460  +  0.40753186d*E (JD2441400 - 44000);
AH    Vir |since JD2444000 - see Table.
AK    Vir |VB B (A = BD -17deg 3996; B 44", 286deg).
AL    Vir |P var [A/H] = -0.7.
AN    Vir |P2 ~1000d is superimposed.
AO    Vir |VB A (B 11.4m vis, 6.9", 321deg, 1956, common
AO    Vir |Vr). delta(M) is possibly in error because of the
AO    Vir |companion. P var. Max = 2413949  +  256.88d*E
AO    Vir |(JD2412900 - 21000); since JD2421000 - see Table.
AS    Vir |P var. The Table gives the mean elements valid after
AS    Vir |JD2425600. Blazhko effect? [03506].
AS    Vir |(k - b)2 = 0.08.
AT    Vir |P var. Max = 2426831.367 + 0.5258053d*E
AT    Vir |(JD2420500 - 35000) [00188]; since JD2435000 - see Table.
AT    Vir |(k - b)2 = 0.00, Delta(S) = 6.0.
AU    Vir |[Fe/H] = -1.84, Delta(S) = 10.1.
AV    Vir |Delta(S) = 5.5.
AW    Vir |Min II 11.67.
AX    Vir |Min II 10.24.
AY    Vir |Maser (H2O).
AZ    Vir |Min II 11.37.
BB    Vir |Blazhko effect?
BC    Vir |P var. Max = 2419922.289 + 0.56451468d*E
BC    Vir |(JD2419900 - 30100); the Table gives current elements.
BD    Vir |P var. Min = 2424971.720 + 2.548410d*E
BD    Vir |(JD2424900 - 32000); since JD2432000 - see Table.
BF    Vir |Min II 10.72. Total eclipses.
BF    Vir |P var. Min = 2416595.67 + 0.64057d:*E (JD2414000 - 19000);
BF    Vir |Min = 2440331.809 + 0.64057631d*E
BF    Vir |(JD2426000 - 41000); since JD2441000 - see Table.
BH    Vir |Min II 10.24. Distortion wave?
BH    Vir |(Delta(V) = 0.04m).
BN    Vir |P var. Max = 2419865.422 + 0.39127585d*E
BN    Vir |(JD2419800 - 28300); since JD2432600 - see Table.
BO    Vir |P var. Max = 2419513.388 + 0.52005916d*E
BO    Vir |(JD2419500 - 33000); since JD2433000 - see Table.
BQ    Vir |P var?
BS    Vir |[Fe/H] = -1.84. Delta(S) = 10.1.
BV    Vir |P var. Max = 2426070.488 + 0.4965803d*E
BV    Vir |(JD2419900 - 28500); since JD2436600 - see Table.
BW    Vir |P var. Max = 2420247.403 + 0.4706660d*E
BW    Vir |(JD2420200 - 26800); since JD2426800 - see Table.
CG    Vir |Min II 10.9.
CK    Vir |[Fe/H] = -2.0.
CM    Vir |d = 0.05P. P var. Min = 2425411.330 + 3.40167d*E
CM    Vir |(JD2423900 - 28400) [00001]; during JD2432200 - 34200 - see
CM    Vir |Table.
CS    Vir |The epoch of Max in B light is given.
CS    Vir |SB (Porb = 1618d). IR excess (4.8 mkm).
CU    Vir |ADS 9152 A (B 11.9m, G1V, 60", 212deg).
CW    Vir |The epoch of min is given.
CX    Vir |The depth of Min II 0.30m.
DK    Vir |According to [10189], P1 = 0.1162d, P2 = 0.1086d.
DK    Vir |(k - b)2 = 0.20.
DL    Vir |SB (Porb = 2286d).
DL    Vir |The spectrum shows the A-component of the eclipsing
DL    Vir |system and the G8III star around which the eclipsing
DL    Vir |system is orbiting.
DM    Vir |Min II 9.49. DII = DI.
DN    Vir |P >= 100d.
DT    Vir |Mu alpha = -0.044s, mu delta = -0.02". SB?
DT    Vir |Rotation period 1.535d [10014], A = 0.05m V.
DV    Vir |Blazhko effect?
EF    Vir |According to [04784], const?, 16.1m pg.
EP    Vir |IR excess (4.8 mkm).
EQ    Vir |SB; [Fe/H] = -0.08; mu alpha = -0.018s, mu delta = -0.09".
EQ    Vir |Min = 2441129.585 + 3.914169D*E + 0.0001803345d*E**2,
EQ    Vir |A = 0.10m V, M - m = 0.40P. Soft X-ray source,
EQ    Vir |lg FX/FV = -2.07.
EW    Vir |P >= 100d.
EX    Vir |P >= 100d.
EY    Vir |P >= 100d.
FF    Vir |The P value for magnetic field variations is given.
FG    Vir |ADS 8471 A (B 13.51m, 25", 352deg, 1909;
FG    Vir |C 11.85m, 74", 195deg, 1909).
FI    Vir |Mu alpha = +0.043s, mu delta = -1.22".
FL    Vir |VB AB (A = 0.76", P = 16A). Both components show flares?
FL    Vir |The range of combined brightness is given.
FL    Vir |Mu alpha = -0.118s, mu delta = +0.26".
FM    Vir |SB2, Porb = 38.324d.
FN    Vir |Mu alpha = -0.064s, mu delta = +0.28". SB?
FN    Vir |X-ray source, LX/Lbol = -3.55.
FO    Vir |Min II 6.67.
FQ    Vir |Deep Min II.
GG    Vir |Multiperiodicity, 0.023d <= P <= 0.083d, A <= 0.02m.
GH    Vir |P var.
GK    Vir |The secondary is a red dwarf (M0 - M6).
GL    Vir |Mu alpha = -0.087s; mu delta = +0.23".
GM    Vir |P ~1.6d/n.
GQ    Vir |Mu alpha = -0.045s, mu delta = -0.44".
GR    Vir |The depth of Min II 0.41m.
GU    Vir |P var. Max = 2439236.36 + 0.466562d*E
GU    Vir |(JD2438100 - 39300); during JD2441300 - 42600 - see Table.
LV    Vir |Type RR: is also possible.
MW    Vir |Type DSCTC: is also possible.
NN    Vir |Type EW: is also possible.
alf   Vir |The Table gives the epoch of Min for the ellipsoidal
alf   Vir |variability and Porb. The depth of Min II up to 0.08m.
alf   Vir |SB 2. e = 0.205 +- 0.004. Apsidal motion: Pi = 108a +- 5a.
alf   Vir |Pulsations: P var, P = 0.17378587d (1908 - 1956);
alf   Vir |since 1956 Max = 2445405.63 + 0.17378680d*E [10181]. A var.
alf   Vir |3 companions according to lunar occultation observations:
alf   Vir |3.1m, 0.0025"; 4.5m, 0.05"; 7.5m, 0.5". Soft X-ray source,
alf   Vir |LX/Lbol = 2.9*10**(-8).
psi   Vir |Binary? (lunar occultations).
R     Vol |P var. Max = 2415238 + 441d*E (JD2394100 - 2418800)
R     Vol |[10143]; since JD2422700 - see Table.
S     Vol |P var. Max = 2415042 + 397.6d*E (JD2415000 - 24200),
S     Vol |Max = 2428880 + 392.1d*E (JD2423000 - 28900),
S     Vol |Max = 2434113 + 401.7d*E (JD2428900 - 34900),
S     Vol |Max = 2434910 + 387.2d*E (JD2434900 - 39200);
S     Vol |since JD2439200 - see Table.
T     Vol |P var. Max = 2413135 + 189.8d*E (JD2413100 - 14600);
T     Vol |Max = 2416870 + 171.8d*E (JD2414600 - 16900);
T     Vol |Max = 2416870 + 176.8d*E (JD2416800 - 24400);
T     Vol |Max = 2424460 + 170.8d*E (JD2424400 - 27200);
T     Vol |Max = 2429925 + 182.3d*E (JD2427200 - 30000);
T     Vol |since JD2440000 see Table.
RX    Vol |P < 20d?
ST    Vol |SP component of a very close pair.
SV    Vol |The shape of the light curve varies.
TX    Vol |Min II 10.5. P var. Min I = 2416789.869 + 5.38845d*E
TX    Vol |(JD2415100 - 26000), Min I = 2431150.345 +
TX    Vol |5.3887d*E (JD2426000 - 31400), Min I =
TX    Vol |2433542.609 + 5.388d*E (JD2431400 - 33600)
TX    Vol |[00001]; since JD2433600 see Table.
R     Vul |P var. Max = 2400169 + 138.3d*E (JD2400100 - 02700),
R     Vul |Max = 2402779 + 136.76d*E (JD2402700 - 19800),
R     Vul |Max = 2419880 + 137.45d*E (JD2419800 - 24400),
R     Vul |Max = 2424413 + 136.76d*E (JD2424400 - 28500
R     Vul |[00960]; Max = 2429331 + 135.9d*E (JD2428500 - 32000)
R     Vul |[00001]; since JD2432000 see Table.
S     Vul |In the region of the open cluster C 1947 + 272 [10123].
S     Vul |P var. Max = 2401772 + 67.37d*E (JD2401760 - 6400),
S     Vul |Max = 2408180 + 67.70d*E (JD2408170 - 14950),
S     Vul |Max = 2415285 + 68.26d*E (JD2415300 - 22800),
S     Vul |Max = 2423468 + 67.72d*E (JD2423450 - 27200),
S     Vul |Max = 2428227 + 68.18d*E (JD2428220 - 31300)
S     Vul |[00761]; Max = 2432775 + 67.51d*E (JD2431300 - 34500)
S     Vul |[10148]; Max = 2437150 + 68.66d*E
S     Vul |(JD2436800 - 39600), Max = 2441507 + 67.344d*E
S     Vul |(JD2439600 - 43000) [10124]; since JD2443000 see Table.
S     Vul |[A/H] = 0.1.
T     Vul |P var. Max = 2419372.151 + 4.435589d*E (JD2409880 - 34000);
T     Vul |since JD2434000 see Table.
V     Vul |Min II 8.65. P var. Min I = 2414912.9 + 74.96d*E
V     Vul |(JD2414900 - 20840),  Min I = 2420909.8 + 75.686d*E
V     Vul |(JD2420900 - 24810), Min I = 2425072.9 + 76.344d*E
V     Vul |(JD2425050 - 30000), Min I = 2430023.5 + 75.957d*E
V     Vul |(JD2430000 - 32500) [10149]. Study of period variation and
V     Vul |changes of Min II by Min I see also in [00767,010150].
W     Vul |In the region of the open clusters NGC 6882, NGC 6885.
X     Vul |P var. Max = 2420636.337 + 6.319301d*E (JD2417000 - 34000)
X     Vul |[00768]; since JD2435000 - see Table.
Z     Vul |VB A (B 12.0m, 13", 359deg). Min II 7.58. P var. Min I =
Z     Vul |2425456.117 + 2.454926d*E (JD2413200 - 37000)
Z     Vul |[00063]; since JD2437000 - see Table.
RS    Vul |Min II 6.86; Min II - Min I = 0.508P.
RU    Vul |A var. P var. Max = 2416266 + 155.95d*E
RU    Vul |(JD2415000 - 36000), Max = 2436779 + 150.7d*E
RU    Vul |(JD2436000 - 38800), Max = 2438855 + 153.4d*E
RU    Vul |(JD2438800 - 41620), Max = 2441193 + 138.5d*E
RU    Vul |(JD2441620 - 42600); since JD2442600 - see Table.
RX    Vul |P var. Max = 2420301 + 438d*E (JD2418900 - 22500)
RX    Vul |[04018]; since JD2424700 - see Table.
RZ    Vul |Slow variations of mean brightness with P = 1410D and
RZ    Vul |A = 2m are superimposed by fluctuations with the cycle
RZ    Vul |40 - 100d and A up to 1m.
SU    Vul |In the region of the open cluster NGC 6882, NGC 6885.
SV    Vul |[Fe/H] = 0.23. P var. There is a nonlinear term in the
SV    Vul |elements given in the Table: -0.0001814d*E**2.
SX    Vul |In the region of the open cluster NGC 6940.
UU    Vul |The co-ordinates are wrong?
UU    Vul |[10156].
VV    Vul |Min II 12.1; d = 0.026P. P var. Min I = 2416670.527 +
VV    Vul |3.411224d*E (JD2416600 - 27500) [00134];
VV    Vul |since JD2426000 - see Table.
VW    Vul |Porb = 0.0731d [10160].
VY    Vul |Min II 14.4:.
WW    Vul |There is quasi-periodicity in light minima with the cycle
WW    Vul |404d.
XZ    Vul |Min II 11.4. P var. Min I = 2426477.525 + 3.0895116d*E
XZ    Vul |(JD2416900 - 36000) [04427]; since JD2436000 - see Table.
AB    Vul |The depth of Min II 0.02m.
AD    Vul |Min II 0.010P.
AF    Vul |Min = 2436545.23  +  0.954d*E (JD2436200 - 900) [03148].
AR    Vul |In the region of the open cluster Stock 1.
AT    Vul |Min II 9.3; d = 0.02P.
AW    Vul |Min II 10.9; d = 0.020P.
AX    Vul |d = 0.018P.
AY    Vul |d = 0.020P. P var. Min hel = 2436128.388 + 2.4124239d*E
AY    Vul |(JD2418500 - 40700); since JD2440700 - see Table.
AZ    Vul |Min II 11.9.
BB    Vul |In the region of the open cluster NGC 6940.
BE    Vul |VB A (BC 11.92m, 50", 320deg). Min II 9.90. P var.
BE    Vul |Min I = 2426144.490 + 1.55205d*E
BE    Vul |(JD2426140 - 28880), Min I = 2430698.203 +
BE    Vul |1.5520442d*E (JD2430690 - 34660), Min I =
BE    Vul |2435340.373 + 1.552052d*E (JD2435340 - 40070);
BE    Vul |since JD2440100 - see Table.
BF    Vul |Elements given in the Table represent well only the bright
BF    Vul |maxima. The fainter maxima are represented by the elements:
BF    Vul |Max = 2427731 + 95.4d*E.
BI    Vul |Min II 14.86. P var? Min I = 2424759.70 + 0.251828d*E
BI    Vul |[00193]; since JD2444750 - see Table.
BN    Vul |Delta(S) = 7. P var. Max = 2414815.759 + 0.5941295d*E
BN    Vul |(JD2414000 - 30000) [00388]; Max = 2434244.333 +
BN    Vul |0.59412538d*E (JD2430000 - 36000) [00616];
BN    Vul |Max = 2438265.386 + 0.59412763d*E (JD2436000 -
BN    Vul |41000) [09009]; since JD2441000 - see Table.
BO    Vul |Min II 10.6. P var. Min I = 2429984.332 + 1.9459123d*E
BO    Vul |(JD2415000 - 30000) [00007]; Min I = 2432379.766 +
BO    Vul |1.9459206d*E (JD2427000 - 35000), since
BO    Vul |JD2435300 - see Table.
BP    Vul |Min II 10.5.
BS    Vul |Min II 11.10.
BT    Vul |d = 0.03P; Min II 12.3.
BU    Vul |P var. Min = 2431006.204 + 0.5689904d*E
BU    Vul |(JD2426500 - 31100) [00001];  since JD2433500 - see Table.
BV    Vul |S 6.5/6-.
BW    Vul |P var. Max = 2424000.171 + 0.20102229d*E
BW    Vul |(JD2424000 - 26500), Max = 2426500.079 +
BW    Vul | + 0.20102933d*E (JD2426500 - 31500), Max =
BW    Vul |= 2432000.054 + 0.20103513d*E (JD2431500 - 41000);
BW    Vul |since JD2441000 - see Table.
CD    Vul |Min II 11.9.
CK    Vul |Max 2331186:. Connected with nebulae. Type NR?
CS    Vul |Min II 13.6.
DR    Vul |Min II 9.19; DII = 0.132P.
DR    Vul |There is apsidal motion with the period 37.8 years.
DR    Vul |Elements given in the Table contain supplementary
DR    Vul |terms: -0.07165d*sin(0.05863deg*E) - 0.00269d*
DR    Vul |*sin(0.11726deg*E).
DR    Vul |Min II = 2440301.7934 + 2.2508645d*E + 0.07165d*
DR    Vul |*sin(0.05863deg*E) - 0.00269d*sin(0.11726deg*E).
DR    Vul |P var? [10185]. The depth of minima varies.
DY    Vul |VB A (B 13.0m V, 14", 300deg).
EH    Vul |P var. Max = 2429609 + 185d*E (JD2429600 - 30600);
EH    Vul |since JD2430800 - see Table.
EP    Vul |S 6.5/5.
EQ    Vul |Min II 12.5; Min II - Min I = 0.31P; DII = 0.050P,
EQ    Vul |dII =  0.010P.
ER    Vul |P var. Min I = 2440182.2593 + 0.69809510d*E
ER    Vul |(JD2433100 - 40200) [08592]; since JD2440100 - see Table.
ER    Vul |7.35m <= Min II <= 7.44m. The shape of the light
ER    Vul |curve and depths of minima vary.
ES    Vul |VB A (B 10.1m, 1.6", 126deg).
ET    Vul |[A/H] = -0.4. P var. Max = 2425110.63 + 54.33d*E
ET    Vul |(JD2422900 - 26600), Max = 2432875.80 + 54.33132d*E
ET    Vul |(JD2432700 - 35430), Max = 2438656.99 + 53.81d*E
ET    Vul |(JD2436050 - 39035), Max = 2439253.55 + 54.24d*E
ET    Vul |(JD2439035 - 40990) [10168]; since JD2441900 - see Table.
EU    Vul |Min II 13.3.
EV    Vul |Min II 11.9. P var. Min I = 2428750.459 + 2.822084d*E
EV    Vul |(JD2428400 - 36400) [04027]; Min I = 2436748.37 +
EV    Vul |2.82220d*E (JD2436380 - 750) [03732]; since
EV    Vul |JD2441500 - see Table.
EX    Vul |d = 0.03P.
EY    Vul |The depth of Min II 0.05m.
FG    Vul |In the region of the open cluster NGC 6940. Star 120.
FG    Vul |The epoch of light minimum is given.
FH    Vul |P var. The elements given in the Table are valid since
FH    Vul |JD2436000.
FK    Vul |Blazhko effect.
FM    Vul |Min II 13.0.
FN    Vul |d = 0.02P; Min II 14.2.
FP    Vul |Min II 15.6.
FQ    Vul |Min II 12.9. Apsidal motion with P = 280 years. Correction
FQ    Vul |of mispints in [04248] see in [04244].
FR    Vul |Probably the period must be doubled.
FS    Vul |Min II 15.2.
FU    Vul |sp component of a close pair.
FW    Vul |Min II 12.9.
FY    Vul |sp component of a close pair. Cycle 30 - 70d [04027].
FZ    Vul |Min II 13.9.
GG    Vul |P var. Max = 2427681.0 + 106.5d*E (JD2427500 - 28850);
GG    Vul |since JD2428850 - see Table.
GH    Vul |P = 2.5d?
GI    Vul |Min II 13.8.
GK    Vul |Red.
GN    Vul |Min II 12.4; d = 0.04P.
GO    Vul |Min II - Min I = 0.515P. The depth of Min II 0.03m.
GP    Vul |Min II 11.2; Min II - Min I = 0.48P.
GQ    Vul |nf component of a close triple group of stars.
GQ    Vul |P var. Max = 2434399.825 + 12.647241d*E (JD2426100 - 38000)
GQ    Vul |[04414]; since JD2444600 - see Table.
GR    Vul |Min II 13.3. The chart in [04244] is wrong.
GT    Vul |Min II 15.8.
GU    Vul |Min II 12.2.
GV    Vul |Probably the period must be doubled. Probably the period
GV    Vul |must be doubled.
HI    Vul |Min II 12.6.
HP    Vul |The depth of Min II 0.04m.
HS    Vul |Min II 14.2.
HU    Vul |Blazhko effect?
HV    Vul |P var. Max = 2437165.449 + 0.419906d*E (JD2437100 - 38670);
HV    Vul |since JD2438670 - see Table. Blazhko effect?
HW    Vul |P var. Max = 2429077.0 + 75.44d*E (JD2427190 - 29080),
HW    Vul |Max = 2429077.0 + 73.94d*E (JD2429070 - 32470);
HW    Vul |since JD2432350 - see Table.
IU    Vul |P var. Max = 2434656 + 320.2d*E (JD2432700 - 37860) [04427];
IU    Vul |since JD2437860 - see Table.
IW    Vul |Min II 13.1.
KN    Vul |Min II 13.4.
KO    Vul |Red.
KS    Vul |Very red.
LT    Vul |Multiperiodicity: P1 = 0.109414d, A1(V) = 0.0234m;
LT    Vul |P2 = 0.11094d, A2(V) = 0.0074m; P3 = 0.1215d,
LT    Vul |A3(V) = 0.0070m (JD2444054 - 096) [10173];
LT    Vul |P1 = 0.109621d, A1(B) = 0.0340m; P2 = 0.093528d,
LT    Vul |A2(B) = 0.0136m (JD2444071 - 465) [10193].
LU    Vul |Nova Vul 1968 N2.
LV    Vul |Nova Vul 1968 N1. VB A (B 18m, 6", 115deg).
LW    Vul |Min II 16.3.
MN    Vul |Min II 16.1; Min II - Min I = 0.518P; DII = 0.10P.
MO    Vul |Min II 14.8. P var?
MR    Vul |P2 = 111.0d?
MT    Vul |Multiperiodicity:
MT    Vul |P2 = 119.93d (A2 = 0.3m), P3 = 25.02d (A3 = 0.4m:).
MX    Vul |P = 181.8d?
NO    Vul |Min II 14.1.
NS    Vul |VB A (B 8.8m, A0, 0.73", 273deg, 1978.6),
NS    Vul |The range of combined light variation is given.
PS    Vul |VB A (B 10.0m, 0.4", 105deg, 1980.0); SB2.
PT    Vul |P1 = 256.12714s (A1 = 1.14%), Max1 =
PT    Vul |2445166.660914 HJED; P2 = 256.33205s (A2 = 1.09%),
PT    Vul |Max2 = 2445166.659424 HJED; P3 = 128.11496s (A3 = 0.37%),
PT    Vul |Max3 = 2445166.660024 HJED. mu = 0.1508", P=1.6deg.
PU    Vul |Pre-outburst SP M4 (1958). Gradual light increase in
PU    Vul |1977 - 79 up to 8.7m V; in 1979 A = 0.29M V,
PU    Vul |Min I = 2443943.39 + 78.12d*E [10197]. In the max of 1979
PU    Vul |Sp F5Ia - F8-9I. In February 1980 an abrupt light decrease
PU    Vul |started; the star reached V = 13.65m by early September.
PU    Vul |By September, 1981 the star recovered from the deep Min of
PU    Vul |500d duration. During the 1980 - 81 minimum Sp M5 with TiO
PU    Vul |bands, emissions of Halpha, NaD, [OII], FeII, rare earths.
PU    Vul |In 1982 - 84 8.35m - 8.87m V, Sp became F again. Simetimes
PU    Vul |Halpha, Hbeta emissions have been detected, often
PU    Vul |with P Cyg profiles.
V0398 Vul |Not identical to IRC+30416 = NSV 12861.
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