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

2005/07/14 by Marco Limongi, Limongi, Marco, A. Chieffi +2
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Pulsars and Gravitational Waves Research #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0507340

6 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

arxiv created 2005/07/14 · openalex publication_date 2005/07/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We present a new analysis of the abundances observed in extremely metal poor\nstars based on both a new generation of theoretical presupernova models and\nexplosions of zero metallicity massive stars and a new abundance analysis of an\nhomogeneous sample of stars having [Fe/H]<-2.5 (Cayrel et al. 2004).\n

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