Asymptotic Giant Branch. Learning outcomes Evolution and internal structure of low mass stars from the core He burning phase to the tip of the AGB Nucleosynthesis.
AGB star intershell abundances inferred from analyses of extremely hot H-deficient post-AGB stars Klaus Werner Institut für Astronomie und Astrophysik.
On the Nature of the Thermal Pulses on the Asymptotic Giant Branch Alessandro Chieffi
