Article contents
Nucleosynthesis of popIII core collapse supernovae and the abundances in extremely metal poor stars
Published online by Cambridge University Press: 23 December 2005
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 $\rm [Fe/H]\leq -2.5$ (Cayrel et al. 2004).
- Type
- Contributed Papers
- Information
- Copyright
- © 2005 International Astronomical Union
- 1
- Cited by