Nucleosynthesis of popIII core collapse supernovae and the abundances in extremely metal poor stars
Abstract
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).
- Publication:
-
From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution
- Pub Date:
- 2005
- DOI:
- 10.1017/S1743921305005867
- Bibcode:
- 2005IAUS..228..303L