Abstract
AGB stars, in particular those of carbon types, are excellent laboratories to constraint the theory of stellar structure, evolution and nucleosynthesis. Despite the uncertainties still existing in the chemical analysis of these stars, the determination of the abundances of several key species in their atmospheres (lithium, s-elements, carbon and magnesium isotopic ratios etc.) is an useful tool to test these theories and the mixing processes during the AGB phase. This contribution briefly review some recent advances on this subject. © 2006 Springer-Verlag Berlin Heidelberg.
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CITATION STYLE
Abia, C., Domínguez, I., Straniero, O., & Zamora, O. (2006). Observational constraints on nucleosynthesis in AGB stars. ESO Astrophysics Symposia, 2006, 23–26. https://doi.org/10.1007/978-3-540-34136-9_6
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