Radiation driven winds with rotation: the oblate finite disc correction factor

We have incorporated the oblate distortion of the shape of the star due to the stellar rotation, which modifies the finite disk correction factor (f D) in the m-CAK hydrodynamical model. We implement a simplified version for the fD allowing us to solve numerically the non-linear m-CAK momentum equat...

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Detalles Bibliográficos
Autores principales:	Araya, Ignacio, Curé, Michel, Granada, Anahí, Cidale, Lydia Sonia
Formato:	Articulo Comunicacion
Lenguaje:	Inglés
Publicado:	2011
Materias:	Ciencias Astronómicas Ciencias Exactas Be Outflows Stars: early-type Stars: emission-line Stars: rotation Stars: winds
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84055
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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