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Nucleosynthesis of popIII core collapse supernovae and the abundances in extremely metal poor stars

Published online by Cambridge University Press:  23 December 2005

M. Limongi  and
A. Chieffi
M. Limongi
Affiliation:
INAF – Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monteporzio Catone (Roma), ITALY email: marco@mporzio.astro.it
A. Chieffi
Affiliation:
INAF – Istituto di Astrofisica Spaziale e Fisica Cosmica, Via Fosso del Cavaliere, I-00133, Roma, ITALY email: achieffi@rm.iasf.cnr.it
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Abstract

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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 $\rm [Fe/H]\leq -2.5$ (Cayrel et al. 2004).

Keywords

Nucleosynthesisstars: abundancesstars: supernovae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S228: From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution , May 2005 , pp. 303 - 308
Copyright
© 2005 International Astronomical Union