Details on Acronym: KeWe | |
KeWe | (Kerber+Weinberger) |
***** | Avoid the usage of KeWe, prefer KW |
Origin | of 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] |
Origin | of the Acronym: D = Assigned by the Dictionary of Acronyms |
Details on Acronym: KW | |
KW | (Kohoutek+Wehmeyer) |
***** | Avoid the usage of KW, prefer [KW2003] |
Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: KW | |
KW | (Kassim+Weiler, 1990) |
***** | Avoid the usage of KW, prefer [KW90] |
Origin | of the Acronym: L (2002RMxAA..38..111O) |
Details on Acronym: KW | |
KW | (Kodaira) |
***** | Avoid the usage of KW, prefer [NVK2008] |
Origin | of 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.+ |
Origin | of 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 |
by | KLEIN 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) |