Super-AGB stars: evolution and associated nucleosynthesis

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dc.creatorPumo, M. L.
dc.creatorSiess, L.
dc.creatorZappala', R. A.
dc.date2008-05-23
dc.date.accessioned2026-07-07T09:40:38Z
dc.date.available2026-07-07T09:40:38Z
dc.descriptionBased on evolutionary computations of 90 stellar models, we have analysed the impact of initial composition and core overshooting on the post-He-burning evolution and the associated nucleosynthesis of Super-AGB stars, pointing particular attention on the C-burning phase. Moreover the possible link between the transition masses $M_{up}$, $M_{N}$ and $M_{mas}$ (defined as the critical initial mass above which C-burning ignites, the minimum initial mass for an electron-capture supernova and the minimum initial mass for the completion of all the nuclear burning phases respectively) and the properties of the core during the core He-burning phase is also briefly discussed.
dc.description4 pages, 2 figures, Proceedings of the ''Catania workshop on nuclear and neutrino astrophysics'', Catania, Italy, February 15-16 2007
dc.identifierhttps://arxiv.org/abs/0805.3611
dc.identifierhttp://arxiv.org/abs/0805.3611
dc.identifierINAF- Catania Astrophysical Observatory Special Publications, 2008, 1, 105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161546
dc.subjectAstrophysics
dc.titleSuper-AGB stars: evolution and associated nucleosynthesis
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