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The most massive AGB stars

Published online by Cambridge University Press:  01 April 2008

Lionel Siess
Lionel Siess*
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles, 1050 Bruxelles, Belgium email: siess@astro.ulb.ac.be Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia
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Abstract

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The general properties of stars in the mass range 7–12M⊙, also referred to as super-AGB stars, are reviewed and special attention is paid to determine how their mass range depends on the initial metallicity and what fraction of these stars end their life as ONe white dwarfs or explode as electron-capture supernova.

Keywords

Stars: AGB and post-AGBstars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 297 - 307
Copyright
Copyright © International Astronomical Union 2008

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