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...
Guardado en:
| Autores principales: | Curé, Michel, Cidale, Lydia Sonia |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2001
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| 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: |
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