Dictionary of Nomenclature of Celestial Objects
(Last update: 19-Apr-2018)

Result of query: info cati W$

Details on Acronym:   OW
   OW (Ohio univ., W stands for 21st hour of RA) ====>Equivalent to: Ohio Originof the Acronym: L = Found in the literature
Details on Acronym:   SMC W
   SMC W (SMC, Westerlund) ***** Avoid the usage of SMC W, prefer [W64] Originof the Acronym: L (1983ApJ...264..114R)
Details on Acronym:   W
   W (Window) ***** Avoid the usage of W, prefer [BBS2005] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Wackering) ***** Avoid the usage of W, prefer CDS Originof the Acronym: L (2001Ap&SS.275..441M)
Details on Acronym:   W
   W (Wilson) ***** Avoid the usage of W, prefer GCRV
Details on Acronym:   W
   W (West) ***** Avoid the usage of W, prefer [GEO97] Originof the Acronym: L (1998ApJ...509..678G)
Details on Acronym:   W
   W (Woolley) ***** Avoid the usage of W, prefer GJ
Details on Acronym:   W
   W (Walter+) ***** Avoid the usage of W, prefer ScoPMS Originof the Acronym: L (1998A&A...332..825S)
Details on Acronym:   W
   W (Westerbork radio telescope) ***** Avoid the usage of W, prefer [TGC96] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Westerhout) Write:<<W NNA>>
<<W NNAN>>
<<W NN(OH)>>
<<W NN(H2O)>> N: 82+ Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:(Nos 1-82).
Format NNA appears for the first times in 1969MNRAS.142..453W for W 49A and B, and in 1972MNRAS.157...31M, for W 51A to W 51H (the authors use minus letters: W 51a to W 51h), W 51I is added in 1994ApJS...91..713M.
Format '51AN' appears for the first time in 1978MNRAS.183..435S (the authors use minus letters). Ref:=1958BAN....14..215W byWESTERHOUT G. Bull. Astron. Inst. Netherlands, 14, 215-260 (1958) A survey of the continuous radiation from the galactic system at a frequency of 1390 Mc/s . o<W NNA> (Nos 1-82) Ref:=1969MNRAS.142..453W byWYNN-WILLIAMS C.G. Mon. Not. R. Astron. Soc., 142, 453-464 (1969) High resolution observations of the radio source W 49. o<W 49A> (Nos 49A, 49B). Ref:=1972MNRAS.157...31M byMARTIN A.H.M. Mon. Not. R. Astron. Soc., 157, 31-40 (1972) High resolution observations of W51. o<W 51A> (Nos W51A to W51H). Ref:=1978MNRAS.183..435S bySCOTT P.F. Mon. Not. R. Astron. Soc., 183, 435-442 (1978) High resolution radio observations of G49.5-0.4 (W521). oauthors use minus letters: W 51e1 and e2 o<W51E1>, <W 51E2>. Ref:=1993ApJ...417..645G byGAUME R.A. , JOHNSTON K.J., WILSON T.L. Astrophys. J., 417, 645-654 (1993) High-resolution centimeter radio continuum and ammonia maser observations of the W 51 region of star formation. oauthors use minus letters: W 51dN and W 51eN o<W 51D1>, <W 51D2>, <W 51E3>, <W 51E4>, <W 51E5> Ref:=1994ApJS...91..713M byMEHRINGER D.M. Astrophys. J., Suppl. Ser., 91, 713-748 (1994) Radio continuum and radio recombination line observations of W 51. oTable 2: <[M94] LL.l-B.bb> N=9, and <[M94] LL.l-B.b aN> N=22. <[M94] 49.5-0.4 aN> = W 51AN (Nos W 51E6, W 51E7, W 51I) are new Ref:=1997ApJ...488..241Z byZHANG Q. , HO P.T.P. Astrophys. J., 488, 241-257 (1997) Dynamical collapse in W51 massive cores: NH_{3} observations. oW 51e8 = W 51E8 o<W 51E8> =E=Catalogue in electronic form as VIII/64 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Westerlund) ***** Avoid the usage of W, prefer [W61b] Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (Westerlund) ***** Avoid the usage of W, prefer [W64] Originof the Acronym: L (2000AJ....119.2214M)
Details on Acronym:   W
   W (White) ***** Avoid the usage of W, prefer [W78] Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (Weedman) ***** Avoid the usage of W, prefer [W85] Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (WATCH catalogue) ***** Avoid the usage of W, prefer WATCH Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   W
   W (Wood) ***** Avoid the usage of W, prefer WBP Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (Weinberger) ***** Avoid the usage of W, prefer Weinberger
Details on Acronym:   W
   W (Weistrop) ***** Avoid the usage of W, prefer Weis
Details on Acronym:   W
   W (Willmer+) ***** Avoid the usage of W, prefer [WFC91] Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (Wichmann+) ***** Avoid the usage of W, prefer [WKS96] Originof the Acronym: L (1999A&A...346..878M)
Details on Acronym:   W
   W (Wolf) ***** Avoid the usage of W, prefer Wolf Originof the Acronym: L = Found in the literature
Details on Acronym:   W
   W (Wray) ***** Avoid the usage of W, prefer Wray
Details on Acronym:   W
   W (Westerbork radio telescope) ***** Avoid the usage of W, prefer WSRTGP Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* Basel 10 W
   Cl* Basel 10 W (Wooden) Write:<<Cl* Basel 10 W NN>> N: 67 Object:*inCl Ref:=1971A&A....13..218W byWOODEN II W.H. Astron. Astrophys., 13, 218-225 (1971) RGU photographic photometry of the galactic clusters K 4 and Ba 10. o<Cl Basel 10>. Table 1: <Cl* King 4 W NNN> (Nos 1-151). Table 2: <Cl* Basel 10 W NN> (Nos 1-67).
Details on Acronym:   Cl* Basel 8 W
   Cl* Basel 8 W (Wagner) Write:<<Cl* Basel 8 W NNN>> N: 153 Object:*inCl Ref:=1971A&A....14..283W byWAGNER R. Astron. Astrophys., 14, 283-292 (1971) The stellar groups Ba 8, Ba 9 and Be 68. o<Cl Basel N> (Nos 8-9). Table 1: <Cl* Basel 8 W NNN> (Nos 1-153). Table 2: <Cl* Basel 9 W NNN> (Nos 1-112). Table 3: <Cl* Berkeley 68 W NNN> (Nos 1-129).
Details on Acronym:   Cl* Basel 9 W
   Cl* Basel 9 W (Wagner) Write:<<Cl* Basel 9 W NNN>> N: 112 Object:*inCl Ref:=1971A&A....14..283W byWAGNER R. Astron. Astrophys., 14, 283-292 (1971) The stellar groups Ba 8, Ba 9 and Be 68. o<Cl Basel N> (Nos 8-9). Table 1: <Cl* Basel 8 W NNN> (Nos 1-153). Table 2: <Cl* Basel 9 W NNN> (Nos 1-112). Table 3: <Cl* Berkeley 68 W NNN> (Nos 1-129).
Details on Acronym:   Cl* Berkeley 68 W
   Cl* Berkeley 68 W (Wagner) Write:<<Cl* Berkeley 68 W NNN>> N: 129 Object:*inCl Ref:=1971A&A....14..283W byWAGNER R. Astron. Astrophys., 14, 283-292 (1971) The stellar groups Ba 8, Ba 9 and Be 68. o<Cl Basel N> (Nos 8-9). Table 1: <Cl* Basel 8 W NNN> (Nos 1-153). Table 2: <Cl* Basel 9 W NNN> (Nos 1-112). Table 3: <Cl* Berkeley 68 W NNN> (Nos 1-129).
Details on Acronym:   Cl* Berkeley 94 W
   Cl* Berkeley 94 W (Wramdemark) ====>Equivalent to: Cl Berkeley 94
Details on Acronym:   Cl* Blanco 1 W
   Cl* Blanco 1 W (Westerlund+) ====>Equivalent to: Cl* Blanco 1 WGL Originof the Acronym: L (1997A&AS..121..213P)
Details on Acronym:   Cl* Collinder 140 W
   Cl* Collinder 140 W (Williams) Write:<<Cl* Collinder 140 W NN>> N: 26 Object:*inCl Ref:=1967MNSSA..26..126W byWILLIAMS P.M. Mon. Notes Astron. Soc. South Africa, 26, 126-127 (1967) The open cluster Cr 140. o<Cl* Collinder 140 W NN> (Nos 1-26).
Details on Acronym:   Cl* IC 2602 W
   Cl* IC 2602 W (Whiteoak) Write:<<Cl* IC 2602 W NNa>> N: 67 Object:*inCl Ref:=1961MNRAS.123..245W byWHITEOAK J.B. Mon. Not. R. Astron. Soc., 123, 245-256 (1961) A study of the galactic cluster IC 2602. I. A photoeletric and spectroscopic investigation. o<Cl* IC 2602 W NNa> (Nos 1-32, 33a, 33b, 34-66) (67-95)
Details on Acronym:   Cl* IC 5146 W
   Cl* IC 5146 W (Walker) ====>Equivalent to: IC 5146
Details on Acronym:   Cl* IC 5146 W
   Cl* IC 5146 W (Walker) Write:<<Cl* IC 5146 W VNN>> N: 21 Object:V* Stat:is completely incorporated in Simbad Ref:=1959ApJ...130...57W byWALKER M.F. Astrophys. J., 130, 57-68 (1959) Studies of extremely young clusters. III. IC 5146. oTables 1, 2, 3: <IC 5146 NN> (Nos 1-76). Table 4: <Cl* IC 5146 W VNN> (Nos V1-V21).
Details on Acronym:   Cl* King 4 W
   Cl* King 4 W (Wooden) Write:<<Cl* King 4 W NNN>> N: 151 Object:*inCl Ref:=1971A&A....13..218W byWOODEN II W.H. Astron. Astrophys., 13, 218-225 (1971) RGU photographic photometry of the galactic clusters K 4 and Ba 10. o<Cl Basel 10>. Table 1: <Cl* King 4 W NNN> (Nos 1-151). Table 2: <Cl* Basel 10 W NN> (Nos 1-67).
Details on Acronym:   Cl* NGC 1039 W
   Cl* NGC 1039 W (Wachmann) Write:<<Cl* NGC 1039 W NNNN>> N: 1367 Object:*inCl Rem:First field of A. A. Wachmann's "Spektral-Durchmusterung
von Milchstrassenfeldern", vol. 1, 1939.
The list is found as:
ftp://ftp.lowell.edu/pub/bas/starcats/bsd.m34 Ref:=1939SDM...B01....0W byWACHMANN A.A. Spektral-Durchmusterung von Milchstrassenfeldern. Teil 1 <Hamburg - Bergedorf (1939)>, 1, 0-None (1939) Spektral-Durchmusterung von Milchstrassenfeldern. o<Cl* NGC 1039 W NNNN> N=1367 among (Nos 1-2521).
Details on Acronym:   Cl* NGC 1039 W39
   Cl* NGC 1039 W39 (Wachmann) ====>Equivalent to: Cl* NGC 1039 W
Details on Acronym:   Cl* NGC 104 W
   Cl* NGC 104 W (Wildey) ====>Equivalent to: NGC 104 Originof the Acronym: L = Found in the literature
Details on Acronym:   Cl* NGC 1502 W
   Cl* NGC 1502 W (Weitenbeck) Write:<<Cl* NGC 1502 W NNa>> N: 75+1 Object:*inCl Ref:=1997AJ....114..222W byWEITENBECK A.J. Astron. J., 114, 222-227 (1997) Cross identification in the region of cluster NGC 1502. oTable 2: <Cl* NGC 1502 W NNa> (Nos 1-75, 58b) =E=Catalogue in electronic form as <J/AJ/114/222/>
Details on Acronym:   Cl* NGC 1851 W
   Cl* NGC 1851 W (Walker) Write:<<Cl* NGC 1851 W NNNNN>> Object:*inCl Ref:=1998AJ....116..220W byWALKER A.R. Astron. J., 116, 220-236 (1998) CCD photometry of galactic globular clusters. IV. The NGC 1851 RR Lyrae variables. oTable 7 : NGC 4499 misprint for IC 4499. oTable 3: <Cl* NGC 1851 W NNNNN> Nos among (Nos 34-10649). Table 5: <Cl* NGC 1851 SAW VNN> (Nos V27-V33) added.
Details on Acronym:   Cl* NGC 1851 Walker
   Cl* NGC 1851 Walker (Walker) Rem:Fom ref. 1998AJ....116..220W ====>Equivalent to: Cl* NGC 1851 W
Details on Acronym:   Cl* NGC 1866 W
   Cl* NGC 1866 W (Walker) Write:<<Cl* NGC 1866 W NNNN>> N: 6556 Object:*inCl Rem:Table 5 Ref:=1995AJ....110..638W byWALKER A.R. Astron. J., 110, 638-645 (1995) The LMC cluster NGC 1866. I. A revised photometric sequence and a reconnaissance of the surrounding field population. oTable 3: <Cl* NGC 1866 AT A> (Nos P-Z). Table 4: <Cl* NGC 1866 RR N> (Nos 1-4). Table 5: <Cl* NGC 1866 W NNNN> N=6556. =E=Catalogue in electronic form as <J/AJ/110/638/>
Details on Acronym:   Cl* NGC 2081 W
   Cl* NGC 2081 W (Westerlund) ====>Equivalent to: NGC 2081
Details on Acronym:   Cl* NGC 2231 W
   Cl* NGC 2231 W (Walker) Write:<<Cl* NGC 2231 W NNN>> N: 134 Object:*inCl Ref:=1979MNRAS.188..735W byWALKER M.F. Mon. Not. R. Astron. Soc., 188, 735-744 (1979) Electronographic photometry of star clusters in the Magellanic Clouds - VII. The colour-magnitude diagram of NGC 2231. oTable 3: <Cl* NGC 2231 W NNN> (Nos 1-134).
Details on Acronym:   Cl* NGC 2257 W
   Cl* NGC 2257 W (Walker) Write:<<Cl* NGC 2257 W NNN>> N: 530 Object:*inCl Ref:=1989AJ.....98.2086W byWALKER A.R. Astron. J., 98, 2086-2123 (1989) CCD photometry of the RR Lyrae variables in the LMC cluster NGC 2257 and the adjacent field. oT.VIII: * VNN = 'Cl* NGC 2257 A VNN', * VNNNN = 'NHU VNNNN' oTable VI: <Cl* NGC 2257 W NNN> (Nos 1-530) =E=Catalogue in electronic form as <J/AJ/98/2086/>
Details on Acronym:   Cl* NGC 2264 W
   Cl* NGC 2264 W (Walker) ====>Equivalent to: NGC 2264
Details on Acronym:   Cl* NGC 2439 W
   Cl* NGC 2439 W (White) ====>Equivalent to: NGC 2439
Details on Acronym:   Cl* NGC 2451 W
   Cl* NGC 2451 W (Williams) ====>Equivalent to: NGC 2451
Details on Acronym:   Cl* NGC 2451 W
   Cl* NGC 2451 W (Williams) Write:<<Cl* NGC 2451 W NNN>> N: 59+29+4 Object:*inCl Ref:=1966MNSSA..25..122W byWILLIAMS P.M. Mon. Notes Astron. Soc. South Africa, 25, 122-131 (1966) Photometry of NGC 2451. oTables I to IV: <Cl* NGC 2451 W NNN> N=59 among (Nos 1-127) + N=29 among (Nos 201-242) + (Noas 981-984).
Details on Acronym:   Cl* NGC 2808 W
   Cl* NGC 2808 W (Walker) Write:<<Cl* NGC 2808 W NN>>
<<Cl* NGC 2808 W A>> N: 23+1 Object:*inCl Rem:N=23 standards in the field of NGC 2808, and
N=1 very Red * (letter 'R'). Ref:=1999AJ....118..432W byWALKER A.R. Astron. J., 118, 432-441 (1999) CCD photometry of galactic globular clusters. V. NGC 2808. o(Erratum) Erratum vol. 119, p. 1512 (2000) oTable 1: <Cl* NGC 2808 W NN> (Nos 1-23). p.435: <Cl* NGC 2808 W A> (No. R).
Details on Acronym:   Cl* NGC 2808 W
   Cl* NGC 2808 W (White) ====>Equivalent to: Cl* NGC 2808 Wh
Details on Acronym:   Cl* NGC 346 W
   Cl* NGC 346 W (Walborn) Write:<<Cl* NGC 346 W N>> N: 6 Object:*inCl Rem:No. 5 missing Ref:=1978ApJ...224L.133W byWALBORN N.R. Astrophys. J., 224, 133-135 (1978) A very early O star in the Small Magellanic Cloud. o<Cl* NGC 346 W N> (Nos 1-2). Ref:=1986ApJ...304L..17W byWALBORN N.R. , BLADES J.C. Astrophys. J., 304, 17-19 (1986) An O3 star in the Small Magellanic Cloud HII region NGC 346. o<Cl* NGC 346 W N> (Nos 3-4) added. Ref:=1995PASP..107..104W byWALBORN N.R. , LENNON D.J., HASER S.M., KUDRITZKI R.-P. Publ. Astron. Soc. Pac., 107, 104-119 (1995) The physics of massive OB stars in different parent galaxies. I. Ultraviolet and optical spectral morphology in the Magellanic Clouds. o<Cl* NGC 346 W N> (No. 6) added.
Details on Acronym:   Cl* NGC 346 WB
   Cl* NGC 346 WB (Walborn+Blades) ====>Equivalent to: Cl* NGC 346 W
Details on Acronym:   Cl* NGC 4103 W
   Cl* NGC 4103 W (Wesselink) ====>Equivalent to: NGC 4103
Details on Acronym:   Cl* NGC 5139 W
   Cl* NGC 5139 W (Woolley) ====>Equivalent to: NGC 5139
Details on Acronym:   Cl* NGC 5927 W
   Cl* NGC 5927 W (White) Write:<<Cl* NGC 5927 W A>> N: 10 Object:*inCl Ref:=1970AJ.....75..167W byWHITE R.E. Astron. J., 75, 167-168 (1970) Secondary UBV comparison stars near some Southern globular clusters. I. Stars brighter than 16th magnitude. oTable II: <Cl* NGC 2808 WH A> (Nos A-M, I missing). Table III: <Cl* NGC 5927 W A> (Nos A-K, I missing). Table IV: <Cl* NGC 6101 W A> (Nos A-S, I and O missing). =E=Catalogue in electronic form as <J/AJ/75/167/>
Details on Acronym:   Cl* NGC 6101 W
   Cl* NGC 6101 W (White) Write:<<Cl* NGC 6101 W A>> N: 17 Object:*inCl Ref:=1970AJ.....75..167W byWHITE R.E. Astron. J., 75, 167-168 (1970) Secondary UBV comparison stars near some Southern globular clusters. I. Stars brighter than 16th magnitude. oTable II: <Cl* NGC 2808 WH A> (Nos A-M, I missing). Table III: <Cl* NGC 5927 W A> (Nos A-K, I missing). Table IV: <Cl* NGC 6101 W A> (Nos A-S, I and O missing). =E=Catalogue in electronic form as <J/AJ/75/167/>
Details on Acronym:   Cl* NGC 6204 W
   Cl* NGC 6204 W (Whiteoak) Write:<<Cl* NGC 6204 W NN>> N: 78 Object:*inCl Rem:1963MNRAS.125..105W: Table II, (Nos 1-78)
1996AJ....111.1609F: Table 2, (Nos 79-96)
Some objects are in Cl Hogg 22, and also named 'Cl* Hogg 22 WhFs' Ref:=1963MNRAS.125..105W byWHITEOAK J.B. Mon. Not. R. Astron. Soc., 125, 105-125 (1963) An association of O and B stars in Ara. oTable I: <[W63] NNN> N=127. Table II: <Cl* NGC 6204 W NN> N=78 Ref:=1996AJ....111.1609F byFORBES D. , SHORT S. Astron. J., 111, 1609-1614 (1996) NGC 6204 and HOGG 22 : the odd couple. oTable 2: <Cl* NGC 6204 W NN> (Nos 79-96), <Cl* Hogg 22 WhFs NNN> (Nos 97-104) and N=20 among (Nos 7-77)
Details on Acronym:   Cl* NGC 6204 Wh
   Cl* NGC 6204 Wh (Whiteoak) ====>Equivalent to: Cl* NGC 6204 W
Details on Acronym:   Cl* NGC 6204 WhFs
   Cl* NGC 6204 WhFs (Whiteoak+Forbes) ====>Equivalent to: Cl* NGC 6204 W
Details on Acronym:   Cl* NGC 6402 W
   Cl* NGC 6402 W (Wehlau) Write:<<Cl* NGC 6402 W A>> N: 17 Object:*inCl Rem:From Wehlau, private communication. Ref:=1979ApJ...228..423M byMOULD J. , STUTMAN D., McELROY D. Astrophys. J., 228, 423-429 (1979) TiO band strengths in metal-rich globular clusters. II. oFig.1a, Table 1: <Cl* NGC 6402 W A> (Nos A-Q). Fig.1b, Table 1: <Cl* NGC 6626 MSM A> (Nos A-H).
Details on Acronym:   Cl* NGC 6611 W
   Cl* NGC 6611 W (Walker) ====>Equivalent to: NGC 6611
Details on Acronym:   Cl* NGC 663 W
   Cl* NGC 663 W (Wallenquist)
Details on Acronym:   Cl* NGC 6791 W
   Cl* NGC 6791 W (Worthey+) Write:<<Cl* NGC 6791 W N>> N: 1 Object:*inCl Ref:=2003PASP..115...96W byWORTHEY G. , JOWETT K.J. Publ. Astron. Soc. Pac., 115, 96-103 (2003) The metal abundances of NGC 188 and NGC 6791 from low-resolution spectra. o<Cl* NGC 6791 W 1> = <NAME WORTHEY 1>
Details on Acronym:   Cl* NGC 7078 W
   Cl* NGC 7078 W (W UMa type) ====>Equivalent to: Cl* NGC 7078 JLK
Details on Acronym:   Cl* NGC 7654 W
   Cl* NGC 7654 W (Wallenquist) Write:<<Cl* NGC 7654 W NNN>> N: 769 Object:*inCl Ref:=1929MeUpp..42....0W byWALLENQUIST A. Uppsala Astr. Obs. Medd., -1-None (1929) A photometric research on two open clusters in Cassiopeia. oTable VII: format NNN' is NNNA in SIMBAD. oTable V: <Cl* NGC 7654 W NNN> (Nos 1-769). Table VII: <NGC 663 NNN> (Nos 1-634), <NGC 663 NNNA> N=28.
Details on Acronym:   Cl* NGC 869 W
   Cl* NGC 869 W (Wildey) Write:<<Cl* NGC 869 W NNNa>> N: 307 Object:*inCl Ref:=1964ApJS....8..439W byWILDEY R.L. Astrophys. J., Suppl. Ser., 8, 439-496 (1964) The stellar content of h and χ Persei cluster and association. oTable 9: <Cl* NGC 869 W NNNa> (Nos 1-307). Table 10: <Cl* NGC 884 W NNNa> (Nos 1-301)
Details on Acronym:   Cl* NGC 884 W
   Cl* NGC 884 W (Wildey) Write:<<Cl* NGC 884 W NNNa>> N: 301 Object:*inCl Ref:=1964ApJS....8..439W byWILDEY R.L. Astrophys. J., Suppl. Ser., 8, 439-496 (1964) The stellar content of h and χ Persei cluster and association. oTable 9: <Cl* NGC 869 W NNNa> (Nos 1-307). Table 10: <Cl* NGC 884 W NNNa> (Nos 1-301)
Details on Acronym:   Cl* Pismis 22 W
   Cl* Pismis 22 W (Westerlund) ====>Equivalent to: Cl Pismis 22
Details on Acronym:   Cl* Ruprecht 79 W
   Cl* Ruprecht 79 W (Walker) ====>Equivalent to: Cl* Ruprecht 79 Walk
Details on Acronym:   Cl* Westerlund 1 W
   Cl* Westerlund 1 W (Westerlund) Rem:Westerlund, 1961 ====>Equivalent to: Cl Westerlund 1
Details on Acronym:   Cl* Westerlund 1 W
   Cl* Westerlund 1 W (Westerlund) Write:<<Cl* Westerlund 1 W NNNa>> N: 88+68+102+5 Object:*inCl Rem:1987A&AS...70..311W:
Table III: (Nos 1-88), stars in the central region of the cluster

Table IV: (Nos 201-268), stars in the outer part of the cluster

Table V: (Nos 301-402), stars in the surrounding of the cluster. Ref:=1987A&AS...70..311W byWESTERLUND B.E. Astron. Astrophys., Suppl. Ser., 70, 311-324 (1987) Photometry and spectroscopy of stars in the region of a highly reddened cluster in Ara. oCluster in Ara = Cl Westerlund 1 oTable III: <Cl* Westerlund 1 W NN> (Nos 1-88). Table IV: <Cl* Westerlund 1 W NNN> (Nos 201-268). Table V: <Cl* Westerlund 1 W NNN> (Nos 301-402). Ref:=2005A&A...436..541N byNEGUERUELA I. , CLARK J.S. Astron. Astrophys., 436, 541-547 (2005) Further Wolf-Rayet stars in the starburst cluster Cl Westerlund 1. oTable 2: <Cl* Westerlund 1 CN A> (Nos O-S) added. Table 2: <WR NNa> (Nos 77a-77s) added. Table 2, Fig. 2: <Cl* Westerlund 1 W NNNa> (Nos 14b, 14c, 46a, 57c) added.

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