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VMS evolutionary tracks
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VMS evolutionary tracks
Evolutionary tracks for 120-500 Msolar with Z=0.014,0.006 and 0.002
P120z06S0.wg
P120z06S4.wg
P120z14S0.wg
P120z14S4.wg
P150z02S4.wg
P150z06S0.wg
P150z06S4.wg
P150z14S0.wg
P150z14S4.wg
P200z02S4.wg
P200z06S4.wg
P200z14S0.wg
P200z14S4.wg
P300z02S4.wg
P300z06S4.wg
P300z14S0.wg
P300z14S4.wg
P500z06S0.wg
P500z06S4.wg
P500z14S0.wg
P500z14S4.wg
tracks.tar.gz
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Very Massive Star Models
README file for evolutionary tracks
VMS evolutionary tracks
P120z06S0.wg
P120z06S4.wg
P120z14S0.wg
P120z14S4.wg
P150z02S4.wg
P150z06S0.wg
P150z06S4.wg
P150z14S0.wg
P150z14S4.wg
P200z02S4.wg
P200z06S4.wg
P200z14S0.wg
P200z14S4.wg
P300z02S4.wg
P300z06S4.wg
P300z14S0.wg
P300z14S4.wg
P500z06S0.wg
P500z06S4.wg
P500z14S0.wg
P500z14S4.wg
tracks.tar.gz
Selected final structure for PCSNe studies
S-process yields from Frischknecht et al 12,16
Convective Boundary Mixing Uncertainties
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