Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars

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dc.creatorLimongi, Marco
dc.creatorChieffi, Alessandro
dc.date2005-07-14
dc.date.accessioned2026-07-07T02:18:16Z
dc.date.available2026-07-07T02:18:16Z
dc.descriptionWe present a new analysis of the abundances observed in extremely metal poor stars based on both a new generation of theoretical presupernova models and explosions of zero metallicity massive stars and a new abundance analysis of an homogeneous sample of stars having [Fe/H]<-2.5 (Cayrel et al. 2004).
dc.description6 pages, 4 figure, Proceedings of the IAU Symp. No. 228 "From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution", V.Hill, P.Francois & F.Primas eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0507340
dc.identifierhttp://arxiv.org/abs/astro-ph/0507340
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9424
dc.subjectAstrophysics
dc.titleNucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars
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