Publications (35)
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
Massive stellar models: rotational evolution, metallicity effects
Sylvia Ekström, Cyril Georgy, Georges Meynet +2
CNO production in first generation stars
Sylvia Ekström, Georges Meynet, André Maeder
Populations of rotating stars III. SYCLIST, the new Geneva Population Synthesis code
Cyril Georgy, Anahi Granada, Sylvia Ekström +5
$s$-process production in rotating massive stars at solar and low metallicities
Urs Frischknecht, Raphael Hirschi, Marco Pignatari +7
Effects of Rotation on Mass Loss for Population III stars
Sylvia Ekström, Georges Meynet, André Maeder
Pre-supernova mixing in CEMP-no source stars
Arthur Choplin, Sylvia Ekström, Georges Meynet +3
Massive star formation by accretion I. Disc accretion
Lionel Haemmerlé, Patrick Eggenberger, Georges Meynet +2
Convective envelopes in rotating OB stars
André Maeder, Cyril Georgy, Georges Meynet
The different progenitors of type Ib, Ic SNe, and of GRB
Cyril Georgy, Georges Meynet, Rolf Walder +2
Massive stars, successes and challenges
Georges Meynet, André Maeder, Cyril Georgy +4
Evolution of surface CNO abundances in massive stars
André Maeder, Norbert Przybilla, Maria Fernanda Nieva +4
Can very massive stars avoid Pair-Instability Supernovae?
Sylvia Ekström, Georges Meynet, André Maeder
Evolution of the Most Massive Stars
André Maeder, Georges Meynet, Raphael Hirschi
The thermohaline, Richardson, Rayleigh-Taylor, Solberg-Hoiland, and GSF criteria in rotating stars
André Maeder, Georges Meynet, Nadège Lagarde +1
Stellar rotation: Evidence for a large horizontal turbulence and its effects on evolution
André Maeder
Wind anisotropy and stellar evolution
Cyril Georgy, Georges Meynet, André Maeder
Effects of Rotation on Presupernovae Models
Georges Meynet, Raphael Hirschi, André Maeder
Initial conditions for reaching the critical velocity
Georges Meynet, Sylvia Ekström, André Maeder +1
Populations of rotating stars. - I. Models from 1.7 to 15 Msun at Z = 0.014, 0.006, and 0.002 with Ω/Ωcrit between 0 and 1
Cyril Georgy, Sylvia Ekström, Anahà Granada +4
The GSF Instability and Turbulence do not Account for the Relatively Low Rotation Rate of Pulsars
Raphael Hirschi, André Maeder
Stellar evolution with rotation and magnetic fields:III: The interplay of circulation and dynamo
André Maeder, Georges Meynet
The basic role of magnetic field in stellar evolution
André Maeder, Georges Meynet, Cyril Georgy +1
Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
Sylvia Ekström, Cyril Georgy, Patrick Eggenberger +9
Clues about the first stars from CEMP-no stars
Arthur Choplin, Georges Meynet, André Maeder
Evolution at very low and zero Z
Georges Meynet, André Maeder, Sylvia Ekström
Chemical Abundances and Yields from Massive Stars
André Maeder, Georges Meynet, Raphael Hirschi
Evolution of massive stars with rotation and mass loss
André Maeder, Georges Meynet
Constraints on CEMP-no progenitors from nuclear astrophysics
Arthur Choplin, André Maeder, Georges Meynet +1
Effects of anisotropic winds on massive stars evolution
Cyril Georgy, Georges Meynet, André Maeder
Massive star formation by accretion II. Rotation: how to circumvent the angular momentum barrier?
Lionel Haemmerlé, Patrick Eggenberger, Georges Meynet +3
Models of rotating massive stars: impacts of various prescriptions
Georges Meynet, Sylvia Ekström, André Maeder +4
Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014
Cyril Georgy, Sylvia Ekström, Georges Meynet +5
On the Eddington limit and WR Stars
André Maeder, Cyril Georgy, Georges Meynet +1
On the Origin of the High Helium Sequence in $Ï$ Centauri
André Maeder, Georges Meynet