Evolution of the Most Massive Stars
| dc.creator | Maeder, André | |
| dc.creator | Meynet, Georges | |
| dc.creator | Hirschi, Raphael | |
| dc.date | 2004-08-18 | |
| dc.date.accessioned | 2026-07-07T02:14:18Z | |
| dc.date.available | 2026-07-07T02:14:18Z | |
| dc.description | We discuss the physics of the $ΩΓ$-- Limit, i.e. when the star is unbound as a result of {\emph{both}} rotation and radiation pressure. We suggest that the $ΩΓ$-- Limit is what makes the Humphreys--Davidson Limit. Stellar filiations are discussed, with an emphasis on the final stages, in particular on the final masses, their angular momentum and the chemical yields with account of rotation. A possible relation between WO stars and GRB is emphasized. | |
| dc.description | 10 pages, 8 figures, in ``The Fate of the Most Massive Stars'', ASP Conf. Series | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0408320 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0408320 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8065 | |
| dc.subject | Astrophysics | |
| dc.title | Evolution of the Most Massive Stars | |
| dc.type | text |