Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati SW$

Details on Acronym:   SW
  
SW (Supper+White)
***** Avoid the usage of SW, prefer [K99]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   SW
  
SW (Sramek+Weedman)
***** Avoid the usage of SW, prefer KP
Originof the Acronym: L (1982ApJ...262..460E)

Details on Acronym:   SW
  
SW (Sarg+Wramdemark)
Write:<<SW NNN>>
N: 150
Object:*  (SIMBAD class: Star)
Stat:is completely incorporated in Simbad
Ref:=1970A&AS....2..251S
bySARG K. , WRAMDEMARK S.
 Astron. Astrophys., Suppl. Ser., 2, 251-259 (1970)
  Photoelectric photometry of early-type stars in a Milky Way field in Cepheus.
o<SW NNN> (Nos 1-150).
Originof the Acronym: L = Found in the literature

Details on Acronym:   Cl* NGC 1850 SW
  
Cl* NGC 1850 SW (Sebo+Wood)
Write:<<Cl* NGC 1850 SW NNNNN>>
N: >10753
Object:*inCl
in source:NAME LMC
Ref:=1995ApJ...449..164S
bySEBO K.M. , WOOD P.R.
 Astrophys. J., 449, 164-177 (1995)
  Variable stars in Magellanic Cloud clusters. II. NGC 1850.
o<Cl* NGC 1850 SW NNNNN> N≥10753
=E=Catalogue in electronic form as <J/ApJ/449/164/>

Details on Acronym:   Cl* NGC 330 SW
  
Cl* NGC 330 SW (Sebo+Wood)
Write:<<Cl* NGC 330 SW NNNN>>
Object:*inCl
Ref:=1994AJ....108..932S
bySEBO K.M. , WOOD P.R.
 Astron. J., 108, 932-943 (1994)
  Variable stars in and around the SMC cluster NGC 330.
oTables 1, 2: <Cl* NGC 330 SW NNNN> N=50 among 8192.
=E=Catalogue in electronic form as <J/AJ/108/932/>

Details on Acronym:   Cl* NGC 4147 SW
  
Cl* NGC 4147 SW (Sandage+Walker)
====>Equivalent to: NGC 4147

Details on Acronym:   Cl* NGC 6341 SW
  
Cl* NGC 6341 SW (Sandage+Walker)
====>Equivalent to: NGC 6341

Details on Acronym:   Cl* NGC 6341 SW
  
Cl* NGC 6341 SW (Sandage+Walker)
Write:<<Cl* NGC 6341 SW xNN>>
N: 22
Object:*inCl
Rem:Table 1: numbering system from earlier studies, given here
for the first time.
Ref:=1966ApJ...143..313S
bySANDAGE A. , WALKER M.F.
 Astrophys. J., 143, 313-326 (1966)
  Three-color photometry of the bright stars in the globular cluster M 92.
oTables 1, 2, 3: <NGC 6341 NN>, <NGC 6341 NNNN>, <NGC 6341 NNNNN> N=147. Table 1: <Cl* NGC 6341 SW XNN> (Nos X1-X22).

Details on Acronym:   Cl* NGC 6356 SW
  
Cl* NGC 6356 SW (Sandage+Wallerstein)
Write:<<Cl* NGC 6356 SW A>>
<<Cl* NGC 6356 SW NNN>>
N: 25+166
Object:*inCl
Ref:=1960ApJ...131..598S
bySANDAGE A. , WALLERSTEIN G.
 Astrophys. J., 131, 598-609 (1960)
  Color-magnitude diagram for the disk globular cluster NGC 6356 compared with halo clusters.
oTable 1: <Cl* NGC 6356 SW A> (Nos A-Y). Table 2: <Cl* NGC 6356 SW NNN> (Nos 1-166).

Details on Acronym:   Cl* NGC 7006 SW
  
Cl* NGC 7006 SW (Sandage+Wildey)
Write:<<Cl* NGC 7006 SW R-NNN>>
N: 108+61
Object:*inCl
Rem:* in ring II and ring III.
Format can also be written 'NNNN' with 4 digits,
ex.: Cl* NGC 7006 SW II-1 = Cl* NGC 7006 SW 2001
Ref:=1967ApJ...150..469S
bySANDAGE A. , WILDEY R.
 Astrophys. J., 150, 469-482 (1967)
  The anomalous color-magnitude diagram of the remote globular cluster NGC 7006.
oTable 2: <Cl* NGC 7006 SW II-NNN> (Nos II-1 to II-108), Cl* NGC 7006 SW III-NN> (Nos III-1 to III-61).