Abstract
It is now recognized that most early-type stars show mass-outflow variability. Using as example the Be stars, we discuss the effects of such variability on the structure of the stellar atmosphere and its implications on stellar modeling.
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© 1988 Kluwer Academic Publishers
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Doazan, V., Thomas, R.N. (1988). Implications of Variable Mass-Outflow on Modeling. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_17
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DOI: https://doi.org/10.1007/978-94-009-2941-8_17
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7824-5
Online ISBN: 978-94-009-2941-8
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