Details on Acronym: Cl* NGC 5139 PKD | |
| Cl* NGC 5139 PKD | (Piotto+King+Djorgovski+) |
| Write: | <<Cl* NGC 5139 PKD NNNNN>> |
| N: | about 14700 |
| Object: | *inCl |
| Ref: | =2005ApJ...621..777P |
| by | PIOTTO G. , VILLANOVA S., BEDIN L.R., GRATTON R., CASSISI S., MOMANY Y., RECIO-BLANCO A., LUCATELLO S., ANDERSON J., KING I.R., PIETRINFERNI A., CARRARO G. |
| Astrophys. J., 621, 777-784 (2005) | |
| Metallicities on the double main sequence of ω Centauri imply large helium enhancement. | |
| o | Table 1: <Cl* NGC 5139 PKD NNNN> N= 34 among (Nos 179-4302). |
| Ref: | =2007ApJ...663..296V |
| by | VILLANOVA S. , PIOTTO G., KING I.R., ANDERSON J., BEDIN L.R., GRATTON R.G., CASSISI S., MOMANY Y., BELLINI A., COOL A.M., RECIO-BLANCO A., RENZINI A. |
| Astrophys. J., 663, 296-314 (2007) | |
| The multiplicity of the subgiant branch of ω Centauri: evidence for prolonged star formation. | |
| o | Tables 1, 2: <Cl* NGC 5139 PKD NNNNN>, N=22+57 among (Nos 145-63840). |
| =E= | Catalogue in electronic form as J/ApJ/663/296 |
Details on Acronym: Cl* NGC 5139 PVB | |
| Cl* NGC 5139 PVB | (Piotto+Villanova+Bedin+) |
| ====> | Equivalent to: Cl* NGC 5139 PKD |
Details on Acronym: Cl* NGC 5139 VPK | |
| Cl* NGC 5139 VPK | (Villanova+Piotto+King+) |
| ====> | Equivalent to: Cl* NGC 5139 PKD |