We present a new set of presupernova evolutions and explosive yields of massive stars of initial solar composition (Y=0.285, Z=0.02) in the mass range 13-35 Msun. All the models have been computed with the latest version (4.97) of the FRANEC code that now includes a nuclear network extending from neutrons to Mo98. The explosive nucleosynthesis has been computed twice: a first one with an hydro code and a second one following the simpler radiation dominated shock approximation (RDA).
@article{arxiv.astro-ph/0304185,
title = {Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae},
author = {M. Limongi and A. Chieffi},
journal= {arXiv preprint arXiv:astro-ph/0304185},
year = {2009}
}
Comments
20 pages, 10 figures, 12 tables. Accepted for publication on ApJ