Evolution of massive stars with rotation and mass loss

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dc.creatorMaeder, André
dc.creatorMeynet, Georges
dc.date2003-01-14
dc.date.accessioned2026-07-07T02:07:10Z
dc.date.available2026-07-07T02:07:10Z
dc.descriptionRotation 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.
dc.description10 pages, 13 figures, IAU Symp. 215 ``Stellar Rotation'', A. Maeder and P. Eenens eds., ASP Conf Ser. in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0301259
dc.identifierhttp://arxiv.org/abs/astro-ph/0301259
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5610
dc.subjectAstrophysics
dc.titleEvolution of massive stars with rotation and mass loss
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