Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity

Alex Camilo Gormaz-Matamala, Jorge Cuadra, Sylvia Ekström +3

We use Geneva-evolution-code to run evolutionary tracks for stellar masses ranging from $20$ to $85$ $M_{\odot }$ at SMC metallicity ($Z=0.002$). We upgrade the recipe for stellar win…