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

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

2005-07-14

arxiv.org/abs/astro-ph/0507340v1

Astronomy and Astrophysics

Astrophysics

6 pages, 4 figure, Proceedings of the IAU Symp. No. 228 "From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution"

Scientific paper

We 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).

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