Saved in:
Bibliographic Details
Main Authors: Van Eck, Sophie, Abia, Carlos, Dominguez, Inma
Format: Preprint
Published: 2026
Subjects:
Online Access:https://arxiv.org/abs/2604.09205
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866914463502827520
author Van Eck, Sophie
Abia, Carlos
Dominguez, Inma
author_facet Van Eck, Sophie
Abia, Carlos
Dominguez, Inma
contents Oxygen and carbon-rich AGB stars - and objects directly polluted by them - are excellent laboratories to investigate the nucleosynthesis and mixing processes occurring during the later phases of the of low- and intermediate-mass star evolution. The determination of the abundances of several s-elements is a key tool for constraining theoretical AGB models. This contribution discusses the main results, recent advances, and current problems on this subject.
format Preprint
id arxiv_https___arxiv_org_abs_2604_09205
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars
Van Eck, Sophie
Abia, Carlos
Dominguez, Inma
Solar and Stellar Astrophysics
Oxygen and carbon-rich AGB stars - and objects directly polluted by them - are excellent laboratories to investigate the nucleosynthesis and mixing processes occurring during the later phases of the of low- and intermediate-mass star evolution. The determination of the abundances of several s-elements is a key tool for constraining theoretical AGB models. This contribution discusses the main results, recent advances, and current problems on this subject.
title Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2604.09205