Evolution of massive stars with rotation and mass loss

Details Evolution of massive stars with rotation and mass loss Evolution of massive stars with rotation and mass loss

2003-01-14

arxiv.org/abs/astro-ph/0301259v1

Astronomy and Astrophysics

Astrophysics

10 pages, 13 figures, IAU Symp. 215 ``Stellar Rotation'', A. Maeder and P. Eenens eds., ASP Conf Ser. in press

Scientific paper

Rotation appears as a dominant effect in massive star evolution. It largely affects all the model outputs: inner structure, tracks, lifetimes, isochrones, surface compositions, blue to red supergiant ratios, etc. At lower metallicities, the effects of rotational mixing are larger; also, more stars may reach critical velocity, even if the initial distribution of rotational velocities is the same.

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