Developments in physics of massive stars
Georges Meynet, Sylvia Ekstrom, Andre Maeder, Raphael Hirschi, Cyril, Georgy, Coralie Beffa
TL;DR
This paper reviews recent advances in the physics of massive stars, emphasizing the importance of rotation, and presents new results from rotating models compared with observational data.
Contribution
It introduces new rotating stellar models and compares them with observations, highlighting rotation as a crucial factor in massive star physics.
Findings
Rotation significantly influences massive star evolution.
New models align better with observational features.
Rotation is confirmed as a key aspect of massive star physics.
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.
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