Massive stellar models: rotational evolution, metallicity effects

The Be star phenomenon is related to fast rotation, although the cause of this fast rotation is not yet clearly established. The basic effects of fast rotation on the stellar structure are reviewed: oblateness, mixing, anisotropic winds. The processes governing the evolution of the equatorial veloci...

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Detalles Bibliográficos
Autores principales:	Ekström, Sylvia, Georgy, Cyril, Meynet, Georges, Maeder, André, Granada, Anahí
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2011
Materias:	Ciencias Astronómicas Ciencias Exactas Be Outflows Stars: emission-line Stars: evolution Stars: mass loss Stars: rotation Stars: winds
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84049
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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