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Supernova Nucleosynthesis in Massive Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 Mʘ to 70 Mʘ 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.
- Type
- Type lb and Type II Supernovae
- Information
- International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 157 - 164
- Copyright
- Copyright © Cambridge University Press 1996