Grids of stellar models with rotation : I. Models from 0.8 to 120 M⊙ at solar metallicity (Z = 0.014)

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. 
\nMethods. We computed a grid of 48 different stellar evolutionary tracks, both rotating and non-rotating, at Z = 0.014, spanning a wide mass range from 0.8 to 120 M⊙. For each of the stellar masses considered, electronic tables…

• NS
  National Science Foundation
• MO
  Ministry of Education, Culture, Sports, Science and Technology
• SN
  Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
• CN
  Centre National de la Recherche Scientifique
• ES
  European Social Fund