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Model Atmospheres of Be Stars
Published online by Cambridge University Press: 14 August 2015
Extract
The basic concept of what a Be star is we owe to Struve (1931). His proposal that these stars are rapidly rotating and have an extended, disc-like, circumstellar envelope is still the basis for all models of Be stars. Unfortunately, progress in understanding the dynamics of Be stars has been painfully slow, a consequence of the very complex nature of the problem. As yet there does not exist a self-consistent unique model of any Be star.
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- VIII. Atmospheric Models
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- Copyright © Reidel 1982
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