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Instabilities in LBVs and WR Stars

Published online by Cambridge University Press:  12 April 2016

Knut Jørgen Røed Ødegaard
Knut Jørgen Røed Ødegaard*
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, N-0315 Oslo, Norway

Abstract

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Using a dynamical stellar code, detailed evolutionary models have been computed that follow the evolution and nucleosynthesis of massive stars from the pre-MS (accretion phase) up to the onset of O-burning. Various instabilities occur during the evolution. As an example, the evolution of a star with maximum mass 120 Mʘ is discussed.

Type
Section V Pulsation
Information
International Astronomical Union Colloquium , Volume 169: Variable and Non-spherical Stellar Winds in Luminous Hot Stars , 1999 , pp. 353 - 356
Copyright
Copyright © Springer-Verlag 1999

References

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