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Developments in Physics of Massive Stars

Published online by Cambridge University Press:  01 December 2007

Georges Meynet
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
Sylvia Ekström
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
André Maeder
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
Raphael Hirschi
Affiliation:
EPSAM, University of Keele, UK email: r.hirschi@epsam.keele.ac.uk
Cyril Georgy
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
Coralie Beffa
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
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Abstract

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New constraints on stellar models are provided by large surveys of massive stars, interferometric observations and asteroseismology. After a review of the main results so far obtained, we present new results from rotating models and discuss comparisons with observed features. We conclude that rotation is a key feature of massive star physics.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

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