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Developments in physics of massive stars

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

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Authors

Georges Meynet

Sylvia Ekström

André Maeder

Cyril Georgy

Coralie Beffa



Abstract

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.

Conference Name Symposium S250: Massive Stars as Cosmic Engines
Acceptance Date Dec 1, 2007
Publication Date Dec 1, 2007
Publicly Available Date Mar 28, 2024
Publisher Cambridge University Press
Pages 147-160
DOI https://doi.org/10.1017/S1743921308020449
Keywords . stars: abundances, early-type, evolution, mass loss, emission-line, Be, rotation; gamma rays: bursts
Publisher URL http://dx.doi.org/10.1017/S1743921308020449

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