Super- and massive AGB stars – IV. Final fates – initial-to-final mass relation

We explore the final fates of massive intermediate-mass stars by computing detailed stellar models from the zero-age main sequence until near the end of the thermally pulsing phase. These super-asymptotic giant branch (super-AGB) and massive AGB star models are in the mass range between 5.0 and 10.0...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2015-01, Vol.446 (3), p.2599-2612
Main Authors: Doherty, Carolyn L., Gil-Pons, Pilar, Siess, Lionel, Lattanzio, John C., Lau, Herbert H. B.
Format: Article
Language:English
Subjects:
Astronomy
Asymptotic giant branch stars
Carbon
Channels
Combustion
Computation
Giant stars
Metallicity
Neutron stars
Supernovae
Supernovas
White dwarf stars
White dwarfs
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