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arxiv: 0802.2805 · v1 · submitted 2008-02-20 · 🌌 astro-ph

Developments in physics of massive stars

classification 🌌 astro-ph
keywords massivemodelsphysicsresultsstarsasteroseismologycomparisonsconclude
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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.

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