Contents of: J/AN/324/437/./notes.dat

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## (from tabmap V6.0 (2016-08-18)) 2024-03-29T09:29:00
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#-- J/AN/324/437 H{alpha} emission stars toward Bulge (Kohoutek+, 2003)
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#---Table: J/AN/324/437/./notes.dat Individual notes  (60 records)
#      Note I2     ---   Note number
#      Text A77    ---   Text of the note
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No|
te|Text
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 1|Near WR 107a (SMSNPL18, Shara et al., 1999AJ....118..390S).
 2|Identical with [DSH99]454-20 (Dufton et al., 1999, Cat. <J/A+AS/139/231>) and
 2| very probably with PM 1-130 (Preite-Martinez, 1988A&AS...76..317P) = RPZM 4.
 3|Identical with V2400 Oph.
 4|Near 393-92.
 5|Near 393-39.
 6|Identical with Terz V348 (Terzan et al., 1982, Cat. <J/A+AS/49/715>).
 7|Near 455-255.
 8|Near 455-254.
 9|Identical with Terz V2687 (Terzan & Gosset, 1991, Cat. <J/A+AS/90/451>).
10|Near Ve 2-50 (Velge, 1957ApJ...126..302V).
11|Near V703 Sco.
12|Probably identical with [GWC93]38 (Gray et al., 1993MNRAS.264..678G).
13|Identical with [RHI84]10-424 (Raharto et al., 1984AnTok..19..469R).
14|Near/in open cluster Collinder 347 (OCl-1039, C 1743-292).
15|Near/in open cluster Collinder 347 (OCl-1039, C 1743-292).
16|Possibly identical with radio source GRS 000.60-00.10.
17|Identical with [RHI84]10-788 (Raharto et al., 1984AnTok..19..469R).
18|Near cluster of stars NGC 6451 (C 1747-302).
19|Possibly identical with infrared source HFE 40
19| (Hoffmann et al., 1971ApJ...170L..89H).
20|Very probably identical with post-AGB star GLMP 676
20| (Garcia-Lario et al., 1997, Cat. <J/A+AS/126/479>).
21|Identical with V589 Sgr.
22|H-alpha variable.
23|Near 521-119.
24|Identical with He 2-294, which was misclassified as PN in Kohoutek (2001,
24| Cat. <IV/24>), Table 3.
25|Near Ve 2-57 (Velge, 1957ApJ...126..302V).
31|He 3-1339.
32|He 3-1444,WRA 15-1745.
33|He 3-1498.
34|MAC 3-608.
35|LSS 4557.
36|WRA 16-355.
37|Ve 1-16, near 521-118.
38|He 3-1551.
39|MAC 3-573; in Trumpler 27 (OCl-1021, C1732-334).
41|394-48. Uncertain identification in van der Hucht et al. (1981,
41| Cat. <III/215>).
42|394-57; faint star with medium H-alpha em. line visible, we agree with Henize
42| (1976ApJS...30..491H) that it is a nova which will be dealt with in a
42| separate paper.
43|521-98.
44|Star to E disturbs.
45|Ve 2-38.
46|He 3-1539. No H-alpha em.line visible.
47|The visible em.line is not H-alpha.
48|The double star having NW and SE components in the centre is obviously
48| LKH 346 and is identical with Th 27-4 (The, 1961CoBos..10....1T). The two
48| components have a distance of about 4.4"; the cross in the finding chart
48| show their mean position. The coordinates given above differ from those of
48| SIMBAD. KW 2 is a new H-alpha em.line star (see Table 1).
49|No H-alpha em. line was visible on three plates taken in 1967 Aug.; the
49| continuum was fainter than that of the star situated 1.6" to SW. On the
49| direct plate taken in 1980 May the variable appeared brighter than this
49| star. The identification given by Lundstrom & Stenholm (1978IBVS.1393....1L)
49| was used.
50|LKH 102 (Herbig, 1957ApJ...125..654H).
51|Star to N disturbs.
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