Post-AGB stars as tracers of AGB nucleosynthesis: An update

Devika Kamath*, Hans Van Winckel

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    8 Citations (Scopus)
    143 Downloads (Pure)

    Abstract

    The chemical evolution of galaxies is governed by the chemical yields from stars, and here we focus on the important contributions from asymptotic giant branch (AGB) stars. AGB nucleosynthesis is, however, still riddled with complexities. Observations from post-asymptotic giant branch (post-AGB) stars serve as exquisite tools to quantify and understand AGB nucleosynthesis. In this contribution, we review the invaluable constraints provided by post-AGB stars with which to study AGB nucleosynthesis, especially the slow neutron capture nucleosynthesis (i.e., the s-process).

    Original languageEnglish
    Article number233
    Pages (from-to)1-12
    Number of pages12
    JournalUniverse
    Volume8
    Issue number4
    DOIs
    Publication statusPublished - Apr 2022

    Bibliographical note

    Copyright © 2022 by the authors. Licensee MDPI, Basel, Switzerland. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

    Keywords

    • Galaxy: stellar content
    • Magellanic clouds
    • neutron-capture processes
    • stars: abundances
    • stars: AGB and post-AGB
    • stars: chemically peculiar
    • techniques: spectroscopy

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