pith. sign in

arxiv: astro-ph/9601017 · v1 · submitted 1996-01-05 · 🌌 astro-ph

AGB Stars: What Should Be Done ?

classification 🌌 astro-ph
keywords doneevolutionshouldstarswhatanalysisbottomburning
0
0 comments X
read the original abstract

We present a review of AGB star evolution, with emphasis on the nucleosynthesis occurring in these stars. In particular, we discuss hot and cool bottom burning, observational constraints, and analysis of meteoritic grains. This paper was presented at the 32nd Liege Colloquium "Stellar Evolution: What Should Be Done ?"

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.