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## (from tabmap V6.0 (2016-08-18)) 2024-04-16T16:45:16 #--------------------------------------------------------------------------- #-- III/43 Luminous Stars in the Southern Milky Way (Stephenson+ 1971) #-------------------------------------------------------------------------- #---Table: III/43/./rem.dat Remarks and Notes (357 records) # LSS I4 --- [1/5132]+= Designation in the catalogue # Text A74 --- Text of remarks; LSS is repeated when the # text is made of several lines ------------------------------------------------------------------------------- LSS|Text ----|-------------------------------------------------------------------------- 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. -------------------------------------------------------------------------------