Nucleosynthesis and molecular processes in evolved stars: from (radio) isotopes to complex molecular nanostructures
Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars also experience strong mass loss, efficiently
Domingo Aníbal
García Hernández
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