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Grids of stellar models with rotation

Astronomy and Astrophysics · 2011 · Vol. 537 · pp. A146–A146
Sylvia EkströmC. GeorgyP. EggenbergerG. MeynetN. MowlavïA. WyttenbachA. GranadaT. DecressinRaphaël HirschiU. FrischknechtC. CharbonnelA. Maeder

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.

Stellar, planetary, and galactic studiesAstro and Planetary ScienceAstrophysics and Star Formation StudiesPhysicsAstrophysicsStarsMetallicityStellar evolutionSupernovaGalaxyAstronomy

Funding

  • National Science Foundation
  • Ministry of Education, Culture, Sports, Science and Technology
  • Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
  • Centre National de la Recherche Scientifique
  • Science and Technology Facilities Council
  • European Social Fund
Citations
1,625
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References
104
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References
Solar System Abundances and Condensation Temperatures of the Elements
The Astrophysical Journal · 2003 · 4,601 citations
Updated Opal Opacities
The Astrophysical Journal · 1996 · 2,886 citations
Mass-loss predictions for O and B stars as a function of metallicity
Astronomy and Astrophysics · 2001 · 1,639 citations
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