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- W148697956 abstract "In AGB stars of low mass and very low metallicity, [Fe/H] < −2, a large abundance of primary 12C obtained by partial He burning in the convective thermal pulse is mixed with the envelope by each third dredge up episode. A progressive amount of primary 22Ne is produced in the He intershell by the conversion of all CNO nuclei to 14N during H-burning shell, followed by double α capture in the thermal pulse. Despite its very low neutron cross section, 22Ne contributes significantly to the production of primary 23Na, 24Mg, 25Mg, 26Mg. These last two are also obtained by α capture on 22Ne. The neutron capture chain starting from 22Ne continues up to iron, creating primary seeds for the s process. Further on, s elements are produced with high efficiency by neutron capture on the primary iron seeds. The third dredge up mixes with the envelope the freshly synthesized primary" @default.
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- W148697956 date "2007-01-01" @default.
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- W148697956 title "Primary production of light and s elements in very metal-poor Asymptotic Giant Branch stars." @default.
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