2016/01/25 by G. Meynet, Meynet, G., C. Georgy +13
Physics and Astronomy · #Stellar, planetary, and galactic studies #Astro and Planetary Science #Astrophysics and Star Formation Studies
paper · pdf · doi:10.48550/arxiv.1601.06532
Key physical ingredients governing the evolution of massive stars are mass\nlosses, convection and mixing in radiative zones. These effects are important\nboth in the frame of single and close binary evolution. The present paper\naddresses two points: 1) the differences between two families of rotating\nmodels, i.e. the family of models computed with and without an efficient\ntransport of angular momentum in radiative zones; 2) The impact of the mass\nlosses in single and in close binary models.\n