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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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| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2008
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57116159010 |
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