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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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Bibliographic Details
Published in:Кинематика и физика небесных тел
Date:2005
Main Author: Marchenko, S.V.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
Subjects:
Plenary Sessions
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79404
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Winds of Wolf−Rayet stars: phenomenology of mass loss / S.V. Marchenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 23-29. — Бібліогр.: 54 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine

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