Grids of stellar models with rotation
Sylvia EkströmGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandC. GeorgyCentre de recherche astrophysique, École Normale Supérieure de Lyon, 46, allée d’Italie, 69384 Lyon Cedex 07, FranceP. EggenbergerGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandG. MeynetGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandN. MowlavïGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandA. WyttenbachGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandA. GranadaGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandT. DecressinGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandRaphaël HirschiAstrophysics group, EPSAM, Keele University, Lennard-Jones Labs, Keele, ST5 5BG, UKU. FrischknechtAstrophysics group, EPSAM, Keele University, Lennard-Jones Labs, Keele, ST5 5BG, UKC. CharbonnelGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, SwitzerlandA. MaederGeneva Observatory, University of Geneva, Maillettes 51, 1290 Sauverny, Switzerland
2011en
ABI
Abstract
Aims. Many topical astrophysical research areas, such as the properties of planet host stars, the nature of the progenitors of different types of supernovae and gamma ray bursts, and the evolution of galaxies, require complete and homogeneous sets of stellar models at different metallicities in order to be studied during the whole of cosmic history. We present here a first set of models for solar metallicity, where the effects of rotation are accounted for in a homogeneous way.
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Cited by 30 references