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Winds, atmosphere and spectral modelling of massive hotstars
Published online by Cambridge University Press: 15 November 2004
Abstract
In this review, we focus on the winds of standard massive starsof spectral types O and B. We introduce the fundamental parametersthat are used to characterize the stellar winds and we describethe various techniques available nowadays to derive the windproperties. The latter are reviewed and interpreted in theframework of the standard theory of line-driven winds.
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- © EAS, EDP Sciences, 2004
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