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arXiv · astro-ph/9706024

Nucleosynthesis in Type II Supernovae

K. Nomoto·M. Hashimoto·T. Tsujimoto·F. -K. Thielemann·N. Kishimoto·Y. Kubo
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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.

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K. Nomoto, M. Hashimoto, T. Tsujimoto, F. -K. Thielemann, N. Kishimoto, Y. Kubo. 1997-06-03. Nucleosynthesis in Type II Supernovae. https://doi.org/10.1016/s0375-9474(97)00076-6

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