TY  - JOUR
A1  - Meynet, G.
A1  - Georgy, C.
A1  - Maeder, A.
A1  - Ekström, S.
A1  - Groh, J. H.
A1  - Barblan, F.
A1  - Song, H. F.
A1  - Eggenberger, P.
T1  - Physics of massive stars relevant for the modeling of Wolf-Rayet populations
JF  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - Key physical ingredients governing the evolution of massive stars are mass losses, convection and mixing in radiative zones. These effects are important both in the frame of single and close binary evolution. The present paper addresses two points: 1) the differences between two families of rotating models, i.e. the family of models computed with and without an efficient transport of angular momentum in radiative zones; 2) The impact of the mass losses in single and in close binary models.
Y1  - 2015
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87971
SP  - 183
EP  - 188
ER  - 
TY  - JOUR
A1  - Georgy, C.
A1  - Ekström, S.
A1  - Hirschi, R.
A1  - Meynet, G.
A1  - Groh, J. H.
A1  - Eggenberger, P.
T1  - Wolf-Rayet stars as an evolved stage of stellar life
JF  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - Wolf-Rayet (WR) stars, as they are advanced stages of the life of massive stars, provide a good test for various physical processes involved in the modelling of massive stars, such as rotation and mass loss. In this paper, we show the outputs of the latest grids of single massive stars computed with the Geneva stellar evolution code, and compare them with some observations. We present a short discussion on the shortcomings of single stars models and we also briefly discuss the impact of binarity on the WR populations.
Y1  - 2015
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88097
SP  - 229
EP  - 232
ER  -