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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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2007
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57130012 |
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