We present the basic properties of the yields of our latest set of presupernova evolution and explosive nucleosynthesis of massive stars in the range between 11 and 120 Msun having solar and zero metallicity.
@article{arxiv.astro-ph/0601198,
title = {Nucleosynthesis In Core Collapse Supernovae},
author = {M. Limongi and A. Chieffi},
journal= {arXiv preprint arXiv:astro-ph/0601198},
year = {2009}
}
Comments
PDF Document, 6 pages, 2 figures. . Proceedings of "Origin of Matter and Evolution of Galaxies (OMEG05): New Horizon of Nuclear Astrophysics and Cosmology". Nov 8-11-2005, Tokyo, Japan