Evolutionary models of metal-rich horizontal branch stars.
Abstract
Summary. A grid of horizontal and post-horizontal branch evolutionary models with heavy metal content appropriate for metal-rich globular clusters is presented. The possibility of putting restraints on mass loss during the red-giant branch phase is briefly discussed.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- March 1977
- DOI:
- 10.1093/mnras/178.4.533
- Bibcode:
- 1977MNRAS.178..533G
- Keywords:
-
- Abundance;
- Globular Clusters;
- Metallic Stars;
- Red Giant Stars;
- Stellar Evolution;
- Stellar Models;
- Atmospheric Composition;
- Stellar Atmospheres;
- Stellar Envelopes;
- Astrophysics