Details on Acronym: P | |
P | (Parker+) |
***** | Avoid the usage of P, prefer PGMW |
Origin | of the Acronym: L = Found in the literature |
Details on Acronym: Parker | |
Parker | (Parker+) |
***** | Avoid the usage of Parker, prefer PGMW |
Origin | of the Acronym: L (1999AJ....118.1684W) |
Details on Acronym: [PGM92] | |
[PGM92] | (Parker+Garmany+Massey+, 1992) |
====> | Equivalent to: PGMW |
Origin | of 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 |
by | PARKER 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. | |
o | Tables 3-6: <PGMW NNNN> (Nos 1001-1522), (Nos 2001-2345), (Nos 3001-3273), (Nos 4001-4089) |
Origin | of the Acronym: L = Found in the literature |