1.7k citations · 2.7k across the 24 of their papers we have counts for
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Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002
Cyril Georgy, Sylvia Ekström, Patrick Eggenberger +11
(shortened) We provide a grid of single star models covering a mass range from 0.8 to 120 Msun with an initial metallicity Z = 0.002 with and without rotation. We discuss the impac…
Close binary evolution I. The tidally induced shear mixing in rotating binaries
H. F. Song, A. Maeder, G. Meynet +3
We study how tides in a binary system induce some specific internal shear mixing, able to substantially modify the evolution of close binaries prior to mass transfer. We construct…
Populations of rotating stars II. Rapid rotators and their link to Be-type stars
A. Granada, S. Ekström, C. Georgy +4
Even though it is broadly accepted that single Be stars are rapidly rotating stars surrounded by a flat rotating circumstellar disk, there is still a debate about how fast these st…
Red supergiants and stellar evolution
Sylvia Ekström, Cyril Georgy, Georges Meynet +2
We review the significant role played by red supergiants (RSGs) in stellar populations, and some challenges and questions they raise for theoretical stellar evolution. We present h…
How the mass-loss rates of red-supergiants determine the fate of massive stars ?
Cyril Georgy, Sylvia Ekström, Hideyuki Saio +3
Mass-loss rates are one of the most relevant parameters determining the evolution of massive stars. In particular, the rates at which the star loses mass during the red-supergiant…