Hot bottom burning and s-process nucleosynthesis in massive AGB stars at the beginning of the thermally-pulsing phase
We report the first spectroscopic identification of massive Galactic asymptotic giant branch (AGB) stars at the beginning of the thermal pulse (TP) phase. These stars are the most Li-rich massive AGBs found to date, super Li-rich AGBs with log ε (Li) ~ 3
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.