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What Can We Learn from Post-AGB Chemical Studies on the AGB 3RD Dredge-Up Phenomena?

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Post-AGB Objects as a Phase of Stellar Evolution

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 265))

Abstract

In this contribution we focus on the remarkably divers detailed chemical patterns observed in post-AGB stars and we address the question whether AGB (nucleosynthetic) evolutionary models can be further constrained by the results on post-AGB stars.

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Author information

Authors and Affiliations

  1. K. U.Leuven, Instituut voor Sterrenkunde, Celestijnenlaan 200B, 3001, Heverlee, Belgium

    Hans van Winckel & Maarten Reyniers

Authors
  1. Hans van Winckel
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  2. Maarten Reyniers
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Editor information

Editors and Affiliations

  1. Nicolaus Copernicus Astronomical Center, Toruń, Poland

    Ryszard Szczerba  & Sławomir K. Górny  & 

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© 2001 Springer Science+Business Media Dordrecht

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van Winckel, H., Reyniers, M. (2001). What Can We Learn from Post-AGB Chemical Studies on the AGB 3RD Dredge-Up Phenomena?. In: Szczerba, R., Górny, S.K. (eds) Post-AGB Objects as a Phase of Stellar Evolution. Astrophysics and Space Science Library, vol 265. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9688-6_39

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  • DOI: https://doi.org/10.1007/978-94-015-9688-6_39

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5758-7

  • Online ISBN: 978-94-015-9688-6

  • eBook Packages: Springer Book Archive

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