Nucleosynthesis in Type II Supernovae

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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