Dictionary of Nomenclature of Celestial Objects
(Last update: 10-May-2024)

Result of query: info cati KW$

Details on Acronym:   KeWe
  
KeWe (Kerber+Weinberger)
***** Avoid the usage of KeWe, prefer KW
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   KW
  
KW (Kap-Herr+Wendker) (Not yet in Simbad)
***** Avoid the usage of KW, prefer [KW72]
Originof the Acronym: D = Assigned by the Dictionary of Acronyms

Details on Acronym:   KW
  
KW (Kohoutek+Wehmeyer)
***** Avoid the usage of KW, prefer [KW2003]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   KW
  
KW (Kassim+Weiler, 1990)
***** Avoid the usage of KW, prefer [KW90]
Originof the Acronym: L (2002RMxAA..38..111O)

Details on Acronym:   KW
  
KW (Kodaira)
***** Avoid the usage of KW, prefer [NVK2008]
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   KW
  
KW (Kerber+Weinberger)= (KeWe)
Write:<<PN KW NN>>
Object:PN  (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:is completely incorporated in Simbad
Note:In 1995, Ann. of the Israel Phys. Soc., vol. 11, p. 193-197, Table 1
Auth.:KERBER F.+
Originof the Acronym: L (Acker+)

Details on Acronym:   Cl* NGC 2632 KW
  
Cl* NGC 2632 KW (Klein-Wassink)
Write:<<Cl* NGC 2632 KW NNN>>
N: 577
Object:*inCl
Ref:=1927PGro...41....1K
byKLEIN WASSINK W.J.
 Publ. Kapteyn Astron. Lab. Groningen, 41, 1-None (1927)
  The proper motion and the distance of the Praesepe cluster.
o<Cl* NGC 2632 KW NNN> (Nos 1-577)