It has been known for decades that s-process elements from Sr to Pb are produced by Asymptotic Giant Branch stars. However only recently, physically-based mixing mechanisms for the formation of C have been proposed. Among them, we aim to verify the robustness of the model of a MHD induced C-pocket formation. In doing that we present results of nucleosynthesis models for low mass AGB stars, developed from the MHD scenario, compared with the isotopic abundance ratios of s-elements from presolar Mainstream SiC grains.
s-Processing from MHD-Induced Mixing and Isotopic Abundances in Presolar SiC Grains
Palmerini S.;Busso M.;Trippella O.;Vescovi D.
2019
Abstract
It has been known for decades that s-process elements from Sr to Pb are produced by Asymptotic Giant Branch stars. However only recently, physically-based mixing mechanisms for the formation of C have been proposed. Among them, we aim to verify the robustness of the model of a MHD induced C-pocket formation. In doing that we present results of nucleosynthesis models for low mass AGB stars, developed from the MHD scenario, compared with the isotopic abundance ratios of s-elements from presolar Mainstream SiC grains.File in questo prodotto:
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