Current models for the evolution of AGB stars

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While the basic properties of AGB stellar evolution are well established, comprehensive observational studies of late phases of intermediate mass stars continue to generate puzzles for current stellar models. Here, I review current techniques to model AGB stars, and I discuss important aspects of current research of AGB (and post-AGB) stellar evolution with a particular focus on how these interrelate.
Invited review, IAU Symp 209 "Planetary Nebulae", November 2001, Canberra, Australia

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