Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae

Astrophysics, abstract
astro-ph/0304185

From: Marco Limongi <marco@mporzio.astro.it>

Date: Thu, 10 Apr 2003 08:45:23 GMT   (484kb)

Authors:
M. Limongi (INAF-Oss. Roma),
A. Chieffi (IASF-CNR)

Comments: 20 pages, 10 figures, 12 tables. Accepted for publication on ApJ

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).

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