Nucleosynthesis in Type II Supernovae

K. Nomoto(1) , M. Hashimoto(2) , T. Tsujimoto(3) , F.-K. Thielemann(4) , N. Kishimoto(1) , Y. Kubo(1) ((1)Department of Astronomy , University of Tokyo , (2)Department of Physics

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Kyushu University (3)National Astronomical Observatory (4)Institut f\"ur Theoretische Physik Universit\"at Basel)

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classification 🌌 astro-ph

keywords massnucleosynthesisodotsupernovayieldsabundancesalphacalculated

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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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Nucleosynthesis in Type II Supernovae

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