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- W2009474215 abstract "Context. Long soft gamma-ray bursts (LGRBs) are usually associated with the death of the most massive stars. A large amount of core angular momentum in the phases preceding the explosion is required to form LGRBs. A very high initial rotational velocity can provide this angular momentum. This velocity strongly influences the way the star evolves: it is mixed in a chemically homogeneous way and evolves directly towards the blue part of the Hertzsprung-Russell (HR) diagram from the main sequence." @default.
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- W2009474215 date "2013-05-30" @default.
- W2009474215 modified "2023-10-18" @default.
- W2009474215 title "Evidence of quasi-chemically homogeneous evolution of massive stars up to solar metallicity" @default.
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- W2009474215 doi "https://doi.org/10.1051/0004-6361/201321282" @default.
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