Showing papers by "Isabelle Baraffe published in 1992"
Journal Article•
TL;DR: In this paper, the s-process nucleosynthesis during the core helium burning phase of massive stars is investigated for various values of the initial metallicity (Z) for models of stars of masses 15, 20 and 30 M with 10 -8 ≤ Z ≤ 0.02.
Abstract: The s-process nucleosynthesis during the core helium burning phase of massive stars is investigated for various values of the initial metallicity (Z). Models of stars of masses 15, 20 and 30 M ⊙ with 10 -8 ≤ Z ≤ 0.02 are calculated from the zero-age main seqence (ZAMS) to the end of core helium burning. An updated nuclear reaction network coupled to the stellar evolution code is used to follow the s-process nucleosynthesis
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