Pulsations in Evolved Massive Stars

The post-main sequence evolution of massive stars still bears many unknowns. In particular, the physical processes involved in triggering enhanced mass-loss or eruptions are yet to be established. In this Chapter, the post-main sequence evolution of massive stars, and the various phases which are we...

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Detalles Bibliográficos
Autor principal:	Kraus, Michaela
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas asteroseismology instabilities stars: oscillations stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167765
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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