Full computation of massive AGB evolution. II. The role of mass loss and cross-sections

Details Full computation of massive AGB evolution. II. The role of mass loss and cross-sections Full computation of massive AGB evolution. II. The role of mass loss and cross-sections

2005-05-11

arxiv.org/abs/astro-ph/0505221v2

Astronomy and Astrophysics

Astrophysics

27 pages (referee format) + 19 figures

Scientific paper

10.1051/0004-6361:20042396

In the course of a systematic exploration of the uncertainties associated to the input micro- and macro-physics in the modeling of the evolution of intermediate mass stars during their Asymptotic Giant Branch (AGB) phase, we focus on the role of the nuclear reactions rates and mass loss. We consider masses 3

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