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

Result of query: info cati PGMW$

Details on Acronym:   P
  
P (Parker+)
***** Avoid the usage of P, prefer PGMW
Originof the Acronym: L = Found in the literature

Details on Acronym:   Parker
  
Parker (Parker+)
***** Avoid the usage of Parker, prefer PGMW
Originof the Acronym: L (1999AJ....118.1684W)

Details on Acronym:   [PGM92]
  
[PGM92] (Parker+Garmany+Massey+, 1992)
====>Equivalent to: PGMW
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   PGMW
  
PGMW (Parker+Garmany+Massey+Walborn)= (P) = (Parker) = [PGM92]
Write:<<PGMW NNNN>>
N: 522+345+273+89
Object:*  (SIMBAD class: Star)
Stat:is completely incorporated in Simbad
Note:The format 'NNNN' is always a 4 digits format.
Table 3: UBV photometry of * in LH 9: (Nos 1001-1522).
Table 4: BV photometry of * in LH 9: (Nos 2001-2345).
Table 5: UBV photometry of * in LH 10: (Nos 3001-3273).
Table 6: BV photometry of * in LH 10: (Nos 4001-4089).
in source:LH 9
in source:LH 10
Ref:=1992AJ....103.1205P
byPARKER J.W. , GARMANY C.D., MASSEY P., WALBORN N.R.
 Astron. J., 103, 1205-1233 (1992)
  The stellar content of LH 9 and 10 (N11) in the LMC: a case for sequential star formation.
oTables 3-6: <PGMW NNNN> (Nos 1001-1522), (Nos 2001-2345), (Nos 3001-3273), (Nos 4001-4089)
Originof the Acronym: L = Found in the literature