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MEASURING THE ROTATION RATES OF WOLF-RAYET STARS FROM LARGE-SCALE WIND VARIABILITY
The rotational velocity of Wolf-Rayet (WR) stars cannot be measured directly from "classical" photospheric absorption lines. However, it can be infered from periodic large-scale wind variability.Afteridentifying a list of WR stars presenting large-scale spectral variability, we have monit...
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| Publié dans: | Revista Mexicana de Astronomía y Astrofísica |
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| Auteurs principaux: | , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Universidad Nacional Autónoma de México
2008
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| Sujets: | |
| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57116159010 |
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