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Winds of Wolf−Rayet stars: phenomenology of mass loss
Population I Wolf–Rayet (WR) stars are the evolved descendants of massive (M ≥ 25M) O-type stars. The dense, fast radiatively-drivenWR winds efficiently hide all vital information about basic characteristics of the stellar cores. Observing binary systems with WR components, we put firm limits on the...
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| Main Author: | |
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| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2005
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| Series: | Кинематика и физика небесных тел |
| Subjects: | |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/79404 |
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