Clumping-corrected mass-loss rates of Wolf-Rayet stars: comparison with the optically thick wind model
Clumping-corrected mass-loss rates of Wolf-Rayet stars lie in the range 0.2–10 x 10 −5 M ⊙ yr −1 . It was found that optically thick wind models can lead to the observed mass-loss rates of WR stars at certain energy supply conditions in the subsonic zone.
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| Veröffentlicht in: | Symposium - International Astronomical Union 1999, Vol.193, p.84-85 |
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| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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| Zusammenfassung: | Clumping-corrected mass-loss rates of Wolf-Rayet stars lie in the range 0.2–10 x 10
−5
M
⊙
yr
−1
. It was found that optically thick wind models can lead to the observed mass-loss rates of WR stars at certain energy supply conditions in the subsonic zone. |
|---|---|
| ISSN: | 0074-1809 |
| DOI: | 10.1017/S0074180900205068 |