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Yellow evolved stars in open clusters
This paper describes a program in which Galactic cluster post-AGBcandidates were first identified and then analyzed for clustermembership via radial velocities, monitored for possible photometricvariations, examined for evidence of mass loss, and classified ascompletely as possible in terms of their basic stellar parameters. Theintrinsically brightest supergiants are found in the youngest clusters.With increasing cluster age, the absolute luminosities attained by thesupergiants decline. It appears that the evolutionary tracks ofluminosity class II stars are more similar to those of class I than ofclass III. Only two superluminous giant star candidates are found inopen clusters.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Pavo |
| Ascensió Recta: | 18h00m21.79s |
| Declinació: | -58°45'41.3" |
| Magnitud Aparent: | 9.231 |
| Moviment propi RA: | -42.6 |
| Moviment propi Dec: | -68.3 |
| B-T magnitude: | 9.99 |
| V-T magnitude: | 9.294 |
Catàlegs i designacions:
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