The "double final fate" of super-AGB stars and its possible consequences for some astrophysical issues

Details The "double final fate" of super-AGB stars and its possible consequences for some astrophysical issues The "double final fate" of super-AGB stars and its possible consequences for some astrophysical issues

2009-02-05

arxiv.org/abs/0902.0913v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, no figures, Proceedings of the "LII congresso della Societa' Astronomica Italiana", Teramo, May 4-8, 2008, to appear

Scientific paper

Super-AGB stars can conclude their evolution either as neon-oxygen white
dwarfs or as electron-capture supernovae. We discuss the possible consequences
of the existence of this "double final fate" in the self-enrichment of globular
clusters and in the nucleosynthesis process of s-nuclei.

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