STRUCTURED STELLAR WINDS
There are various, but indirect evidences that the radiation-driven winds from hot stars (O-type and Wolf- Rayet) are not homogeneous. Clumping is discussed as an example that a ects the integrated spectra, and thus the mass-loss diagnostics. To resolve structured winds, interferometers might be th...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2010
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57115706018 |
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