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

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dc.creatorPumo, M. L.
dc.creatorVentura, P.
dc.creatorD'Antona, F.
dc.creatorZappala', R. A.
dc.date2009-02-05
dc.date.accessioned2026-07-07T12:38:14Z
dc.date.available2026-07-07T12:38:14Z
dc.descriptionSuper-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.
dc.description4 pages, no figures, Proceedings of the "LII congresso della Societa' Astronomica Italiana", Teramo, May 4-8, 2008, to appear in Mem. S.A.It
dc.identifierhttps://arxiv.org/abs/0902.0913
dc.identifierhttp://arxiv.org/abs/0902.0913
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218690
dc.subjectSolar and Stellar Astrophysics
dc.titleThe "double final fate" of super-AGB stars and its possible consequences for some astrophysical issues
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