arXiv · astro-ph/0507340
Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of 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).
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Marco Limongi, Alessandro Chieffi. 2005-07-14. Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars. https://arxiv.org/abs/astro-ph/0507340
Cite the original work for its findings. Save a collection to share your selection of sources.