Nucleosynthesis in Type II Supernovae

Abstract

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, $^{12}C(α, γ) ^{16}O}$ rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

1 Page Latex source, 10 PostScript figures, to appear in Nuclear Physics A, Vol. A616 (1997)

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