Wind-Blown Bubbles and HII Regions around Massive Stars
Mass loss dominates the evolution of very massive stars, although the mass loss rates are not known exactly,particularly once the star has left the main sequence. Studies of the ring nebulae and HI shells that surroundmany Wolf-Rayet (WR) and luminous blue variable (LBV) stars provide some informati...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2007
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57130012 |
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