Very Large Array Observations of Winds from Massive Stars
The classical model for free-free emission from ionized stellar winds is basedon the assumption of a stationary, isotropic and homogeneous wind. However, sincethere exist objects whose wind behavior deviates from the standard model, theseassumptions have been questioned in the last decade. In this w...
Guardat en:
| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2004
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57140106 |
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