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Cited by 1,051

The DOI matches its Crossref record; 122 of the 122 references it cites were found in a registry or an index.

Evolution of Asymptotic Giant Branch Stars

Herwig, Falk·2005·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract The current status of modeling the evolution and nucleosynthesis of asymptotic giant branch (AGB) stars is reviewed. The principles of AGB evolution have been investigated in recent years leading to improved and refined models, for example with regard to hot-bottom burning or the third dredge-up. The postprocessing s-process model yields quantitative results that reproduce many observations. However, these and most other processes in AGB stars are intimately related to the physics of stellar mixing. Mixing in AGB stars is currently not well-enough understood for accurate yield predictions. Several constraints and methods are available to improve the models. Some regimes of AGB evolution have not yet been studied in sufficient detail. These include the super-AGB stars and AGB stars at extremely low or ultra low metallicity.

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Metadata

Authors
Herwig, F.
Venue
Annual Review of Astronomy and Astrophysics
Published
2005-09-01
Volume
43
Issue
1
Pages
435-479
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2114908771
Cited by
1,051
References
122
FWCI
3.28
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Evolution of Asymptotic Giant Branch Stars. https://app.cochat.ai/papers/10.1146/annurev.astro.43.072103.150600
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Herwig, F. (2005). Evolution of Asymptotic Giant Branch Stars. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.43.072103.150600

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.