Nucleosynthesis in Type II Supernovae
Astrophysics
2009-10-30 v1
Abstract
Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 to 70 are calculated. We examine the dependence of the supernova yields on the stellar mass, ^{12}C(\alpha, \gamma) ^{16}O} rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.
Cite
@article{arxiv.astro-ph/9706024,
title = {Nucleosynthesis in Type II Supernovae},
author = {K. Nomoto and M. Hashimoto and T. Tsujimoto and F. -K. Thielemann and N. Kishimoto and Y. Kubo},
journal= {arXiv preprint arXiv:astro-ph/9706024},
year = {2009}
}
Comments
1 Page Latex source, 10 PostScript figures, to appear in Nuclear Physics A, Vol. A616 (1997)