New constraints on the major neutron source in low-mass AGB stars
New constraints on the major neutron source in low-mass AGB stars
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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We compare updated Torino postprocessing asymptotic giant branch (AGB) nucleosynthesis model calculations with isotopic compositions of mainstream SiC dust grains from low-mass AGB stars. Based on the data-model comparison, we provide new constraints on the major neutron source, 13C({\alpha},n)16O in the He-intershell, for the s-process. We show th...
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New constraints on the major neutron source in low-mass AGB stars
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TN_cdi_proquest_journals_2092784692
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2092784692
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1808.03614
