Vientos MHD en estrellas tempranas
As a part of a modeling plan for early type stars winds which considers its dynamic structure, thermal flux and the system's stability, we present in this paper the basic concepts of the origin of the problem as well as some preliminary results of the MHD winds.
Guardado en:
| Autores principales: | , , , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1992
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/143627 |
| Aporte de: |
| Sumario: | As a part of a modeling plan for early type stars winds which considers its dynamic structure, thermal flux and the system's stability, we present in this paper the basic concepts of the origin of the problem as well as some preliminary results of the MHD winds. |
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