Nucleosynthesis in type II supernovae

K. Nomoto, M. Hashimoto, T. Tsujimoto, F. K. Thielemann, N. Kishimoto, Y. Kubo, N. Nakasato

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Abstract

Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M to 70 M are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ)16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

Original languageEnglish
Pages (from-to)79-90
Number of pages12
JournalNuclear Physics A
Volume616
Issue number1-2
DOIs
Publication statusPublished - Apr 14 1997

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All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

Cite this

Nomoto, K., Hashimoto, M., Tsujimoto, T., Thielemann, F. K., Kishimoto, N., Kubo, Y., & Nakasato, N. (1997). Nucleosynthesis in type II supernovae. Nuclear Physics A, 616(1-2), 79-90. https://doi.org/10.1016/S0375-9474(97)00076-6