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- W3103708186 abstract "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 that the literature Ni, Sr, and Ba grain data can only be consistently explained by the Torino model calculations that adopt the recently proposed magnetic-buoyancy-induced 13C-pocket. This observation provides strong support to the suggestion of deep mixing of H into the He-intershell at low 13C concentrations as a result of efficient transport of H through magnetic tubes." @default.
- W3103708186 created "2020-11-23" @default.
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- W3103708186 date "2018-09-27" @default.
- W3103708186 modified "2023-10-06" @default.
- W3103708186 title "New Constraints on the Major Neutron Source in Low-mass AGB Stars" @default.
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- W3103708186 doi "https://doi.org/10.3847/1538-4357/aad9f3" @default.
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