The main purpose of this lecture is a re-examination of the yields of s-elements by massive short-lived stars. He-burning conditions are reviewed and results are presented for the nucleosynthesis in this phase. The authors briefly analyse the possibility of n-captures during carbon burning and discuss the contribution of massive stars to the enrichment of the interstellar medium in s-elements.
On the production of heavy neutron-rich isotopes during He and C burning in massive stars
BUSSO, Maurizio Maria;
1986
Abstract
The main purpose of this lecture is a re-examination of the yields of s-elements by massive short-lived stars. He-burning conditions are reviewed and results are presented for the nucleosynthesis in this phase. The authors briefly analyse the possibility of n-captures during carbon burning and discuss the contribution of massive stars to the enrichment of the interstellar medium in s-elements.File in questo prodotto:
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