Showing papers on "Stellar nucleosynthesis published in 1971"
116 citations
TL;DR: In this paper, the character of the nuclear abundances synthesized under explosive carbon, oxygen and silicon burning conditions is demonstrated to be dependent upon the initial metal content of the star Specifically, for metal-poor stars, the calculated abundances both of odd-Z nuclei and of the neutron rich isotopes of even Z nuclei are substantially reduced.
Abstract: The character of the nuclear abundances synthesized under explosive carbon, oxygen and silicon burning conditions is demonstrated to be dependent upon the initial metal content of the star Specifically, for metal-poor stars, the calculated abundances both of odd-Z nuclei and of the neutron rich isotopes of even-Z nuclei are found to be substantially reduced This odd-even effect inZ is consistent with spectral studies of metal deficient stars
27 citations
TL;DR: In this paper, the final abundances of the major nuclei produced in explosive, but partial, carbon-burning taking place in a rapidly expanding medium were analyzed and the effects of energy deposition due to burning and expansive cooling were taken into account.
Abstract: Results are presented which show the final abundances of the major nuclei produced in explosive, but partial, carbon-burning taking place in a rapidly expanding medium. the effects of energy deposition due to burning and expansive cooling are taken into account explicity. The results are compatible with those obtained by other authors but show the sensitivity of the final abundances to the assumed initial conditions. A conjecture is made as to the physical site of the burning.
2 citations
DOI•
31 Oct 1971
TL;DR: Radioactive abundances and stable products in chronological model for galactic heavy element nucleosynthesis in this article, which is based on the same model as the one used in this paper.
Abstract: Radioactive abundances and stable products in chronological model for galactic heavy element nucleosynthesis
1 citations