Dictionary of Nomenclature of Celestial Objects
(Last update: 11-Mar-2024)

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 NNaNN>>
<<W NNW(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, W 51i is added in 1994ApJS...91..713M.
Format '51aN' appears for the first time in 1978MNRAS.183..435S.
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>
Ref:=2016A&A...595A..27G
byGINSBURG A. , GOSS W.M., GODDI C., GALVAN-MADRID R., DALE J.E., BALLY J., BATTERSBY C.D., YOUNGBLOOD A., SANKRIT R., SMITH R., DARLING J., KRUIJSSEN J.M.D., LIU H.B.
 Astron. Astrophys., 595A, 27-27 (2016)
  Toward gas exhaustion in the W51 high-mass protoclusters.
oFig. 2, Table 3: <W 51aNN> (Nos W 51d3-d7, W 51e9-e23) added. Figs 2+A.2, Tables 3-8: <[GGG2016] arc> N=1, <[GGG2016] W51aNNw> (Nos W51d3, W51d4e-W51d4w, W51d5-W51d7, W51e8n-W51e8s, W51e9-23), <[GGG2016] W51aNNd> (Nos W51d3d, W51e11d, W51e18d), <[GGG2016] W51aNNmol> (Nos W51e8mol, W51e10mol).
=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.