Nucleosynthesis in AGB Stars
M. Busso
Abstract
Open-access reader
M. Busso
Abstract
Open-access reader
I review some of the main nucleosynthesis processes in Asymptotic Giant Branch (AGB) Stars. These include production of $^{12}$ C, $^{19}$ F, $^{22}$ Ne and $s$ -elements in the He-rich layers above the degenerate C-O core, and modifications in the abundances of intermediate-mass elements up to Mg-Al, due to proton captures above the H-burning shell. Emphasis is put on the uncertainties still affecting the yields (especially mixing processes and mass loss rates) and on the possible role of planetary nebulae as a source of information on the evolution and nucleosynthesis of the AGB progenitors
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I review some of the main nucleosynthesis processes in Asymptotic Giant Branch (AGB) Stars. These include production of $^{12}$ C, $^{19}$ F, $^{22}$ Ne and $s$ -elements in the He-rich layers above the degenerate C-O core, and modifications in the abundances of intermediate-mass elements up to Mg-Al, due to proton captures above the H-burning shell. Emphasis is put on the uncertainties still affecting the yields (especially mixing processes and mass loss rates) and on the possible role of planetary nebulae as a source of information on the evolution and nucleosynthesis of the AGB progenitors
Key concepts: Nucleosynthesis, Asymptotic giant branch, Physics, Planetary nebula, Stellar nucleosynthesis, Stars, Astrophysics, Stellar evolution