Presents a grid of 113 fast-rotating, chemically-homogeneous massive star models at Z=0.001 reaching core collapse with high angular momentum for use as supernova and GRB progenitors.
Erratum: “Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions” <A href="/abs/2015ApJS..220...15P">(2015, ApJS, 220, 15)</A>
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A grid of fast-rotating, chemically-homogeneous, supernova and/or long-GRB progenitors
Presents a grid of 113 fast-rotating, chemically-homogeneous massive star models at Z=0.001 reaching core collapse with high angular momentum for use as supernova and GRB progenitors.