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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| container_title | Symposium - International Astronomical Union |
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| creator | Nugis, Tiit |
| description | 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. |
| doi_str_mv | 10.1017/S0074180900205068 |
| format | Article |
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−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.</abstract><doi>10.1017/S0074180900205068</doi><tpages>2</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0074-1809 |
| ispartof | Symposium - International Astronomical Union, 1999, Vol.193, p.84-85 |
| issn | 0074-1809 |
| language | eng |
| recordid | cdi_crossref_primary_10_1017_S0074180900205068 |
| source | Alma/SFX Local Collection |
| title | Clumping-corrected mass-loss rates of Wolf-Rayet stars: comparison with the optically thick wind model |
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