Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Sep-2023)

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