9 OB?
   38 HR 2284=ADS 4978 AB. USE C.D. FOR CHART.
   56 SOME INDICATION OF DOUBLE LINES ON ONE PLATE.
   90 P CYGNI-LIKE?
   94 CSV.
  104 BRIGHT STAR CATALOGUE NOTES "VAR?",PROBABLY ON BASIS OF PUBLS.ASTRON.SOC.P
  104 ACIFIC 46,233,1934.
  119 P CYGNI-LIKE?
  147 SLIGHT INDICATION OF P CYGNI CHARACTER.
  167 HR 2678=ADS 5795 AB.
  193 MAY BE B7 II.
  202 ADS 5837 A.
  289 DOUBLE LINES?
  355 STRENGTH OF BALMER JUMP ON ONE PLATE SUGGESTS SHELL STAR. NOT IN THE HALF-
  355 EMISSION CATALOGUE OF WACKERLING(1970).A SR-EU STAR ACCORDING TO L.MUNCH,B
  355 OL.OBS.TONANTZINTLA Y TACUBAYA NO.5,WITHOUT PAGE NUMBERS.
  370 DOUBLE LINES?
  391 MWC 560.SPECTRUM NOVA-LIKE WHEN OBSERVED AT MT.WILSON IN 1943; OUR MATERIA
  391 L SUGGESTS THE SPECTRUM MAY BE LITTLE CHANGED 25 YEARS LATER.AT THIS DISPE
  391 RSION THE SPECTRUM RESEMBLES THAT OF NO.1411.
  396 WEAKLY P CYGNI-LIKE.
  418 HR 2855.
  455 PART OF A SMALL ASSOCIATION OF LATE-TYPE SUPERGIANTS,WITH NOS.456,460,AND
  455 463.
  456 SEE 455.
  460 SEE 455.
  463 SEE 455.
  484 DOUBLE.COMPANION ABOUT 10" SOUTH IS ALSO OB+.
  521 A HELIUM-RICH STAR ACCORDING TO MACCONNELL ET AL,PUBLS,ASTRON.SOC.PACIFIC
  521 82,730.
  548 HR 2911. HBET WEAK.
  584 WEAKLY P CYGNI-LIKE.
  591 BLUE PLATE SUGGESTS A POSSIBLE SPECTRAL OVERLAP OF AN OB + WR,BUT THE RED
  591 PLATE DOES NOT CONFIRM.
  603 OVERLAP.
  664 A CLOSE OVERLAP OF TWO STARS,BOTH PROBABLY OB.
  688 OUR LUMINOSITY CLASSIFICATIONS FOR THIS STAR SCATTER CONSIDERABLY BETWEEN
  688 FOUR DIFFERENT PLATES,FROM CLASS III TO IA+,SUGGESTING SHELL ACTIVITY.
  704 HR 2996.
  742 FLAT CONTINUUM.
  766 HBET AND 4686 EMISSION SUSPECTED.
  779 PROBABLY COMPOSITE,OB + M.
  827 INVOLVED IN NEBULOSITY.
  840 APPEARS TO SHOW 4686 EMISSION BUT NO HALF EMISSION.
  868 4686,PLUS THE BALMER SERIES TO HBET OR HGAM,IN EMISSION.
  952 HE I LINES?
  968 USE C.D. FOR CHART.
  980 SDS A,GAM2 VEL.
  983 SDS A.
 1046 H AND K WEAKLY PRESENT?
 1047 H AND K WEAKLY PRESENT?
 1058 SDS AB.
 1078 ONE PLATE INDICATES A2 I.
 1085 SDS AB.
 1094 HD 72754. SEE I.A.U. VAR.STAR INFO.BULL.NO.483.
 1113 HR 3445=SDS A;COMPANION TO 1112.SPECTRUM APPEARS EXCEPTIONALLY HIGH-LUMINO
 1113 SITY,LIKE THE BRIGHTEST SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD.BIDELMAN
 1113  NOTES IN PUBLS.ASTRON.SOC.PACIFIC 66,250 THAT IT APPEARS TO BE SOMEWHAT M
 1113 ORE LIMINOUS THAN THE F2 IA STANDARD STAR 89 HER.
 1166 USE C.D. FOR CHART.
 1179 POSSIBLE SHELL STAR ON BASIS OF HUGE BALMER JUMP.D LINES SUSPECTED ON RED
 1179 PLATE.NOT CONTAINED IN WACKERLING'S CATALOGUE OF HALF-EMISSION STARS,SO TH
 1179 E EMISSION IS PERHAPS VARIABLE.SLIT SPECTROGRAM CONFIRMS SHELL CHARACTER;
 1179 SEE ASTROPHYS.LETTERS,2,153.
 1181 HR 3527=SDS AB.
 1222 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 1310 WEAKLY P CYGNI-LIKE.
 1325 SUSPICION OF G BAND ON ONE PLATE.
 1341 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 1349 RATHER FLAT CONTINUUM.
 1354 PROBABLY SHOWS BLAMER JUMP.
 1365 HR 3920.
 1366 APPEARS TO BE IN A COMPACT CLUSTER WHICH ALSO CONTAINS AN M SUPERGIANT.
 1411 HD 87643.EXTREME P CYGNI TYPE AT OUR DISPERSION,OR,MORE ACCURATELY,NOVA-LI
 1411 KE. SEE ASTROPHYS.LETTERS,2,153.
 1444 CLOSE DOUBLE,OR COMPOSITE,WITH AN M-TYPE PROBABLE LONG-PERIOD VARIABLE.
 1457 HBET IN EMISSION AND POSSIBLY ALSO 4686.
 1475 HD 89249. SEE ASTROPHYS.LETTERS,2,153.
 1481 NO.21 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 1555 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 1625 THIS APPEARS TO BE HD 91421=NO.24 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (
 1625 1962),ENTERED THERE BECAUSE REPORTED AS WN5 BY HOFFLEIT (1956) ALTHOUGH NO
 1625 T CONFIRMED AS SUCH BY US,BY THE HEIDELBERG SURVEY,OR BY SMITH (1968).
 1669 IN NGC 3293,TOO CROWDED TO SHOW ON MAIN IDENTIFICATION CHART.THIS CLUSTER
 1669 IS ONE OF THE RICHEST OB CLUSTERS IN OUR ENTIRE SURVEY,AND ON OUR PLATES A
 1669 PPEARS MAINLY AS A DENSE MASS OF HOPELESSLY OVERLAPPED OB SPECTRA.AS MENTI
 1669 ONED IN THE TEXT,THE ONLY STARS CATALOGUED BY US IN SUCH CASES ARE THOSE F
 1669 EW FOR WHICH IT SEEMS CERTAIN THAT A SINGLE IDENTIFIABLE STAR IS INVOLVED.
 1671 IN NGC 3293.
 1672 IN NGC 3293.
 1674 IN NGC 3293.
 1676 C.P.D. -57 3526.
 1679 IN NGC 3293.
 1685 IN NGC 3293.
 1688 IN NGC 3293.
 1712 SEE I.A.U. CIRCULAR 2328.
 1715 ONE PLATE SUGGESTS POSSIBLE INTERSTELLAR 4430 ABSORPTION.
 1749 COMPOSITE ACCORDING TO THE HD CATALOGUE.
 1759 HBET AND 4686 EMISSION SUSPECTED ON SOME BLUE PLATES (THIS STAR APPEARS ON
 1759 SEVEN OF THERM).
 1765 THE CLASSIFICATION IS PURELY FORMAL,REFLECTING A RECORD-BREAKING BLAMER JU
 1765 MP.PROBABLY A SHELL STAR,ON THIS BASIS.THIS IS HDE 305483=MWC 210 (BE). SE
 1765 E ALSO HARVARD BULL.NO.846,8.
 1839 SDS A.
 1841 NO.1 IN THE LIST OF MACCONNELL AND SANDULEAK (1970).
 1850 DESIGNATED LS 4 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 1932 4686 EMISSION SUSPECTED ON OUR PLATE.CALLED OE5 IN THE HD.FEAST ET AL IN M
 1932 EM.ROY.ASTRON.SOC.68,1,1957 NOTE: "PICKERING SERIES STRONG IN ABSORPTION,B
 1932 UT 4686 NOT SEEN".
 1964 NO.3 IN THE LIST OF MACCONNELL AND SANDULEAK (1970).
 1970 HD 94305=NO.30 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).THE HD RIGHT
 1970 ASCENSION IS 0M.7 IN ERROR.
 2008 OVERLAP IN UV.
 2015 BLUE PLATES SHOW NARROW BALMER EMISSION PLUS OTHER LINES,AND SUGGEST POSSI
 2015 BLE TIO BANDS,THE LATTER NOT CONFIRMED BY THE RED PLATE. PERHAPS THE OBJEC
 2015 T DISCUSSED BY HENIZE IN ASTROPHYS.J.115,133.
 2018 FLAT CONTINUUM.
 2033 SPECTRUM IS SIMILAR TO THAT OF AG CAR,NO.2035.PERHAPS THIS IS THE STAR REF
 2033 ERRED TO BY E.C. PICKERING IN ASTROPHYS.J.4,142,AS SIMILAR TO ETA CARINAE.
 2035 THE BLUE-REGION SPECTRUM IS SIMILAR TO THAT OF GG CAR,NO.2033. THE HALF PL
 2035 ATE,HOWEVER,SHOWS IN ADDITION THAT THERE IS A PLANETARY NEBULA HERE,LISTED
 2035  ALSO BY PEREK AND KOHOUTEK (1967).
 2063 NO.32 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962)? L.SMITH (1968) CALLS
 2063 THIS STAR WN8 + OB.
 2076 NO.33 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 2110 COMPONENT A IS ALSO OB OR OB1.
 2112 DESIGNATED LS 6 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 2148 COMPOSITE?
 2151 FLAT CONTINUUM,WITH VERY WEAK 4686 EMISSION.CONSIDERABLY SIMILAR TO SCO X-
 2151 1;SEE ASTROPHYS.LETTERS 1,247,1968 AND 8,3,1971.
 2158 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2173 DESIGNATED LS 7 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 2182 VERY FLAT CINTINUUM.
 2218 MAY BE CLOSE NORTH-SOUTH DOUBLE.
 2237 HR 4352=SDS A.
 2238 STRONG FEATURE AT THE POSITION OF THE K LINE.
 2268 OVERLAP IN UV.
 2275 LOOKS SOMEWHAT NEBULOUS ON OUR PLATES.
 2289 NO.39 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 2297 PRECEDING STAR OF A PAIR.
 2305 IT IS RATHER SURPRISING THAT THIS RAHTER BRIGHT STAR,THOUGH NOT A KNOWN VA
 2305 RIABLE,IS NOT IN THE HD CATALOGUE.
 2330 MIDDLE STAR IN A ROUW OF THREE.
 2369 HR 4438; OVERLAP.
 2400 SAME NOTE AS FOR 2305.
 2427 SDS ABC.
 2455 POSSIBLY COMPOSITE,WITH A K STAR.
 2457 NO.68 ON CHART BY LYNGA (1969).
 2481 NO.74 ON CHART BY LYNGA (1969).
 2512 NO.87 ON CHART BY LYNGA (1969).
 2513 NO.88 ON CHART BY LYNGA (1969).
 2533 CLASSIFIED ONLY FROM AN HALF PLATE.BELOW THE LIMIT OF THE WURZBURG CHART;
 2533 OUR IMAGE THERE IS HAND-ENTERED.
 2538 SAME REMARK AS 2533.
 2541 COMPOSITE?
 2557 RATHER FLAT CONTINUUM.
 2581 COMPONENT B OF 2580.
 2648 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2652 USE C.D. FOR CHART.
 2672 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2676 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2681 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2682 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2683 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2685 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 2720 HR 4806=SDS A.
 2742 STRONG ABSORPTION NEAR POSITION OF K LINE.
 2744 FOLLOWS A MUCH BRIGHTER STAR BY ABOUT 50".
 2764 WEAK-LINE F STAR?
 2777 PRECEDES A SOMEWHAT BRIGHTER STAR BY 30".
 2933 SDS AB; THE MUSCAE.
 2979 PRECEDING MEMBER OF A 15" PAIR OF SIMILAR BRIGHTNESS.
 3006 ABOUT 15" NORTH PRECEDING A VISUALLY BRIGHTER STAR.
 3038 HR 5027; RATHER FLAT CONTINUUM.
 3071 USE C.D. FOR CHART.
 3076 NORTH FOLLOWING,AND SOUTH PRECEDING,TWO BRIGHTER STARS,BY ABOUT 1/2' IN EA
 3076 CH CASE.
 3085 MIDDLE STAR OF CLOSE STRING OF THREE ALIGNED IN POSITION ANGLE 135-315.
 3108 A FEW SECONDS SOUTH PRECEDING A CONSIDERABLY BRIGHTER STAR.
 3111 NO.48 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 3117 DESIGNATED LS 8 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 3162 NO.51 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 3164 CLASSIFICATION BASED ONLY ON HALF PLATE. ABOUT 10" WEST OF A CONSIDERABLY
 3164 BRIGHTER STAR.
 3166 WR + OB,OR OF.
 3169 BROAD EMISSION BAND IN ULTRAVIOLET? PROBABLY A MONOCHROMATIC IMAGE OF THE
 3169 OTHERWISE UNNOTICED PLANETARY NEBULA NO.309-4.1 OF PEREK AND KOHOUTEK (196
 3169 7).
 3173 NO.52 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962).
 3189 WR + OB,OR OF. CHARTED ON REGION "R".
 3218 GREATLY ENHANCED HBET.
 3219 USE C.D. FOR CHART.
 3231 HR 5375=SDS A. USE C.D. FOR CHART.
 3234 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS.
 3235 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS.
 3239 COMPONENT B OF 3240.
 3268 RATHER FLAT CONTINUUM.
 3289 CLASSIFICATION BASED ONLY ON HALF PLATES.
 3299 LISTED AS PROBABLE WOLF-RAYET WACKERLING (1970).
 3319 CLASSIFICATION BASED ONLY ON HALF PLATE. BELOW THE LIMIT OF THE WURZBURG C
 3319 HART; OUR IMAGE THEREON IS HAND-ENTERED.
 3331 HR 5664.
 3333 CLASSIFICATION BASED ONLY ON HALF PLATE. BELOW THE LIMIT OF THE WURZBURG C
 3333 HART; OUR IMAGE THEREON IS HAND-ENTERED.
 3336 SDS A.
 3347 HE I LINES VISIBLE. HEPS ENHANCED.
 3385 ABOUT 25" EAST OF A COMPARABLY BRIGHT STAR.
 3391 WEAK 4686 EMISSION. SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS. WEBSTER (PUB
 3391 LS.ASTRON.SOC.PACIFIC 78,136,1966) HAS OBSERVED THE 4686 EMISSION ON A SLI
 3391 T SPECTROGRAM.
 3417 COMPONENT B OF THE DOUBLE MAY ALSO BE OB-.
 3418 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS. THIS IS HD 141969 (PROBABLY P CY
 3418 GNI TYPE)=MWC 238? OUR PLATES SHOW BLAMER LINE EMISSION PLUS A STRONG EMIS
 3418 SION NEAR LAM 3727,PRESUMABLY FROM THE ASSOCIATED PLANETARY NEBULA (OTHERW
 3418 ISE UNNOTED BY US) NO.320-9.1 OF THE LIST OF PEREK AND KOHOUTEK (1967).
 3438 USE C.D. FOR CHARTS.
 3464 ALSO BALMER LINE EMISSION,WITH STEEP DECREMENT.
 3465 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS.
 3508 ABOUT 50" NORTH PRECEDING A MUCH BRIGHTER STAR.
 3516 ABOUT 30" SOUTH PRECEDING A BRIGHT STAR.
 3517  ABOUT 1/2' NORTHWEST OF A BRIGHTER STAR. SEE SPECIAL CHARTS FOLLOWING THE
 3517  MAIN CHARTS.
 3531 HEPS ENHANCED.
 3556 ABOUT 40" SOUTH PRECEDING A CONSIDERABLY BRIGHTER STAR.
 3560 ABOUT 50" WEST OF A BRIGHTER STAR.
 3583 ABOUT 30" SOUTH PRECEDING A COMPARABLY BRIGHT STAR.
 3591 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS.
 3606 SEE SPECIAL CHARTS FOLLOWING MAIN CHARTS.
 3636 HR 6142=SDS A.
 3646 CENTRAL STAR OF A PLANETARY NEBULA (NGC 6309) VISIBLE OF THE HALF PLATE.
 3673 SHELL? THE HYDROGEN LINES ARE TOO WEAK FOR THE ASSIGNED TYPE, BUT THERE IS
 3673  NO EVIDENCE OF LINE EMISSION.
 3693 CLASSIFICATION BASED ONLY ON HALF PLATE. BELOW THE LIMIT OF THE WURZBURG C
 3693 HART; OUR IMAGE THERE IS HAND-ENTERED.
 3694 SLIGHT CHANCE OF BEING FP OR F + OB.
 3700 COMPONENT C TO 3701.
 3701 SDS AB.
 3709 A LONG-PERIOD VARIABLE,PROBABLY CSV 2778,IS ABOUT 1/2' TO THE NORTHEAST.
 3741 4686 EMISSION SUSPECTED.
 3764 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3771 30" SOUTH PRECEDING A BRIGHTER STAR.
 3787 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3807 HR 6261.
 3828 SDS A.
 3832 ABOUT 30" SOUTH FOLLOWING A NEARLY EQUAL STAR.
 3853 ABOUT 30" NORTH PRECEDING 3854,WITH WHICH IT IS BLENDED ON THE IDENTIFICAT
 3853 ION CHART.
 3854 SEE REMARK FOR 3853.
 3858 SOUTH FOLLOWING A MUCH BRIGHTER STAR.
 3867 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3871 CLASSIFICATION BASED ONLY ON HALF PLATE.BELOW THE LIMIT OF THE WURZBURG CH
 3871 ART; OUR IMAGE THEREON IS HAND-ENTERED.
 3885 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3888 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3892 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3893 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3896 DESIGNATED LS 11 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 3899 TYPE OF IN WACKERLING (1970).
 3901 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3909 SEE SPECIAL CHARTS FOLLOWING THE MAIN ONES.
 3918 HDE 326823. RATHER LIKE NO.1411. SEE M.N. 122,247.
 3919 HR 6347.
 3937 THIS C.D. STAR IS NOT ON THE C.D. CHART; WOULD OTHERWISE BE CALLED -40 111
 3937 76NP.
 3951 DESIGNATED LS 12 IN THE WOLF-RAYET CATALOGUE OF SMITH (1968).
 3982 A TRIPLE STAR IN THE SDS CATALOGUE. THE PRIMARY IS A G SUPERGIANT,SEE I.A.
 3982 U.CIRC.NO.2143,1969. COMPONENT C IS NOT DETECTABLE ON OUR PLATES.
 4005 CLASSIFICATION BASED ONLY ON AN HALF PLATE.BELOW THE LIMIT OF THE WURZBURG
 4005  CHART;OUR IMAGE THEREON HAS BEEN HAND-ENTERED.
 4064 NEAR NO.4065 (ALSO WR) AND 4067 (OF OR WR + OB). ALL ARE PART OF A CLUSTER
 4064  CONTAINING A NUMBER OF HALF-EMISSION STARS.
 4065 SEE 4064.
 4067 MAY BE WR + OB. SEE 4064.
 4068 PROBABLY ROBERTS (1962) NO.70,THOUGH SMITH (1968) GIVES A DECLINATION 5 DI
 4068 FFERENT.
 4080 ENVELOPED,WITH NOS.4081,4095,AND 4101,IN NEBULOSITY.
 4081 SEE 4080.
 4095 SEE 4080.
 4101 SEE 4080.
 4168 P CYGNI-LIKE.
 4225 SDS A.
 4226 COMPANION (13" IN 80) TO 4225,UNRESOLVED ON IDENTIFICATION CHART.
 4265 CLASSIFICATION BASED ONLY ON HALF PLATES.
 4295 MAY BE F STAR;OVERLAP IN VIOLET.
 4332 HD 160529=MWC 266. OE5 IN HD. THE SPECTRUM IS PERHAPS VARIABLE. SEE ALSO A
 4332 STROPHYS.J.91,592, AND 99,206.
 4334 STRONG EMISSION NEAR HGAM--(0 111)4363?
 4338 FLAT CONTINUUM. THIS IS HD 160641,EXTREMELY HYDROGEN-DEFICIENT (CF. BIDELM
 4338 AN,ASTROPHYS.J.116,227,1952).
 4340 NEAR MAXIMUM WHEN THE HALF PLATES WERE TAKEN;SEE I.A.U.INF.BULL.ON VAR.STA
 4340 RS NO.323,1968.
 4356 CSV.
 4368 SHOWS O VI 3811,3834.THIS STAR WAS ERRONEOUSLY SUGGESTED TO BE THE X-RAY S
 4368 OURCE GX 3+1 IN ASTROPHYS.J.LETTERS 152,L137.
 4394 BLENDED WITH 4393 ON IDENTIFICATION CHART.
 4401 ABOUT 30" SOUTH PRECEDING A SOMEWHAT BRIGHTER STAR,THE PAIR BEING UNRESOLV
 4401 ED ON THE CHART.
 4405 HDE 316285=C.D. -27 11944 (NOT INCLUDED ON C.D. CHART)=MWC 272. MANY EMISS
 4405 ION LINES ARE SEEN ON OUR PLATES,BUT NOT THE EXTREME P CYGNI CHARACTER COM
 4405 MENTED ON BY MERRILL IN PUBLS.ASTRON.SOC.PACIFIC 60,381 AND ASTROPHYS.J.61
 4405 ,418. SEE ALSO ASTROPHYS.J.93,352.MERRILL'S DESCRIPTION OF THE STAR INDICA
 4405 TES THAT NOS.1411 AND 3918 OF THE PRESENT CATALOGUE ARE STILL MORE EXTREME
 4405 . THE REDNESS NOTED BY US FOR NO.4405 HAS LONG BEEN A SOURCE OF INTEREST A
 4405 ND IS APPARENTLY AT LEAST IN LARGE PART INTERSTELLAR SINCE THE LIGHT OF TH
 4405 E STAR SHOWS MORE THAN 3% POLARISATION,SEE ASTROPHYS.J.124,43.
 4430 SDS A.
 4467 ABOUT 25" NORTH PRECEDING A CONSIDERABLY BRIGHTER STAR.
 4478 HBET WEAK.
 4569 PROBABLY NO.80 IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962),ALTHOUGH OUR
 4569 COORDINATES AND HIS ARE UNUSUALLY DISCORDANT.THE POSITION GIVEN BY US IS T
 4569 HE MEAN OF ACCORDANT MEASUREMENTS ON TWO HALF PLATES;THE CLASSIFICATION AL
 4569 SO DEPENDS SOLELY ON THE HALF REGION. THE STAR IS BELOW THE LIMIT OF THE W
 4569 URZBURG CHART,BUT EASILY FOUND ON THE PALOMAR PRINT,WHERE IT IS COMPARABLE
 4569  TO THE BRIGHTER STAR SEVERAL MINUTES TO THE SOUTH. EVIDENTLY THIS STAR IS
 4569  VERY RED.
 4570 SEE 4571.
 4571 ADS 10991 AB,POSITION ANGLE NEARLY PARALLEL TO OUR SPECTRAL DISPERSION.DOU
 4571 BLE LINES SUSPECTED ON ONE PLATE.WITH NO.4570,AT THE CENTER OF A NEBULA.
 4573 OVERLAP IN THE ULTRAVIOLET.HBET EMISSION?
 4574 OBSCURED BY NEBULOSITY ON OUR CHART;USE THE C.D. FOR CHART.
 4575 OBSCURED BY NEBULOSITY ON OUR CHART;USE THE C.D. FOR CHART.
 4580 HR 6727.
 4589 FLAT CONTINUUM. THIS STAR IS USUALLY CALLED HERSCHEL 36, AND IS NEAR THE "
 4589 HOURGLASS"(CF.MONTLY NOT.ROY.ASTRON.SOC.110,343)IN THE NEBULA M8.
 4624 ADS 11024 AB.
 4628 NO.82(WC7) IN THE WOLF-RAYET CATALOGUE OF ROBERTS (1962),ALTHOUGH OMITTED
 4628 FROM THE CATALOGUE OF JASCHEK ET AL (1964).
 4632 HD 165019,CALLED KO IN THE HD CATALOGUE. THIS SPECTRAL CLASSIFICATION DISA
 4632 GREEMENT IS UNUSUAL ALTHOUGH IN A DIRECTION COMMON FOR HD CLASSIFICATIONS
 4632 OF F AND G SUPERGIANTS.
 4637 PRESUMABLY THE STAR DESIGNATED LS 14 (WN + OB) IN THE WOLF-RAYET CATALOGUE
 4637  OF SMITH (1968).OUR DECLINATION,BASED ON ACCORDANT MEASUREMENTS OF FOUR P
 4637 LATES, DIFFERS 8' FROM HERS BUT AGREES WITH THAT OF WACKERLING (1970) IF T
 4637 HE STAR IS INDEED HDE 313846 (OF).
 4654 C.D. -23 13906, NOT PLOTTED ON C.D. CHART. IS NORTH FOLLOWING -23 13908, W
 4654 HICH IS PLOTTED.
 4666 HR 6762.
 4683 A PECULIAR ABSORPTION-LIKE FEATURE NEAR LAM 4700 SUGGEST OB + R, BUT THE R
 4683 ED PLATE DOES NOT CONFIRM.
 4697 SPECTRUM BADLY CONFUSED BY A SECOND, EQUAL STAR 30" SOUTH,WHICH MAY ALSO B
 4697 E UV-RICH. THE OVERLAP MAY HAVE VITIATED THE CLASSIFICATION.
 4710 C.D. -24 13985, NOT PLOTTED ON C.D. CHART.
 4723 OVERLAP WITH 4724.
 4724 OVERLAP WITH 4723.
 4743 ADS 11136 A.
 4750 ADS 11140 AB.
 4757 HD 166612/3, CALLED F5 + A IN HD.
 4769 ADS 11146 AB.
 4790 ADS 11169 B; TOO CLOSE TO THE 3D-MAG.PRIMARY, OUR NO.4791,TO SHOW ON CHART
 4790 . A TO B=16" IN 255.
 4791 13 MU SGR=ADS 11169 A.
 4819 ADS 11191 AB.
 4821 ADS 11193 A.
 4831 HR 6825=ADS 11196 A.
 4973 A HELIUM-RICH STAR ACCORDING TO MACCONNELL ET AL,PUBLS.ASTRON.SOC.PACIFIC
 4973 82,730.
 5132 USE C.D. FOR IDENTIFICATION CHART.