Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-06-03
Astronomy and Astrophysics
Astrophysics
1 Page Latex source, 10 PostScript figures, to appear in Nuclear Physics A, Vol. A616 (1997)
Scientific paper
10.1016/S0375-9474(97)00076-6
Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 $M_\odot$ to 70 $M_\odot$ 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.
Hashimoto Makoto
Kishimoto Nobu
Kubo Yoshio
Nomoto Ken
Thielemann Friederich-Karl
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