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- W2039853826 abstract "Red supergiants (RSG) are a crucial phase in the evolution of massive stars. At solar metallicity, they represent the stage where substantial amounts of mass and angular momentum are lost. Here we investigate the role of RSGs at very low metallicity. We have computed evolutionary tracks at Z=0.0004 with and without rotation, using the latest version of the Geneva stellar evolution code. Here, we briefly discuss the evolution of RSGs, their lifetimes, mass ranges for forming RSGs, maximum luminosity of RSGs, and how these are affected by rotation." @default.
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- W2039853826 date "2013-01-01" @default.
- W2039853826 modified "2023-09-23" @default.
- W2039853826 title "The evolution of Red Supergiants at very low metallicity" @default.
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- W2039853826 doi "https://doi.org/10.1051/eas/1360005" @default.
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