Influence of magnetic in Be-stars disk formation due to rotation in line driven in stellar winds

Line driven wind theory has been improved including non-spherical expansion in order to study its influence upon disk formation in early-type stars. Assuming that magnetic field controls the flow geometry, the plasma must flow downstream through open magnetic field lines. It is found that in the pol...

Descripción completa

Detalles Bibliográficos
Autores principales: Curé, Michel, Cidale, Lydia Sonia
Formato: Articulo
Lenguaje:Inglés
Publicado: 2001
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/2085
http://articles.adsabs.harvard.edu//full/2001ASPC..248..415C/0000415.000.html
Aporte de:SEDICI (UNLP) de Universidad Nacional de La Plata Ver origen

Ejemplares similares