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Developments in Physics of Massive Stars

Meynet, Georges ; Ekström, Sylvia ; Maeder, André ; Hirschi, Raphael ; Georgy, Cyril ; Beffa, Coralie

In: Proceedings of the International Astronomical Union, 2007, vol. 3, no. S250, p. 147-160

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    Titre
    • Developments in Physics of Massive Stars
    Auteur
    • Meynet, Georges. Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
    • Ekström, Sylvia. Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
    • Maeder, André. Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
    • Hirschi, Raphael. EPSAM, University of Keele, UK email: r.hirschi@epsam.keele.ac.uk
    • Georgy, Cyril. Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
    • Beffa, Coralie. Observatory of Geneva University, Switzerland email (G. Meynet): georges.meynet@obs.unige.ch
    Type de document
    • Postprint
    Langue
    • Anglais
    Publié dans
    • Proceedings of the International Astronomical Union, 2007, vol. 3, no. S250, p. 147-160. Cambridge University Press
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:298924
    Summary
    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