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Stellar Models and Yields of Asymptotic Giant Branch Stars
Open accessAbstract
We present stellar yields calculated from detailed models of low and intermediate-mass asymptotic giant branch (AGB) stars. We evolve models with a range of mass from 1 to 6 M⊙, and initial metallicities from solar to 1/200th of the solar metallicity. Each model was evolved from the zero age main sequence to near the end of the thermally pulsing (TP) AGB phase, and through all intermediate phases including the core He-flash for stars initially less massive than 2.5 M⊙. For each mass and metallicity, we provide tables containing structural details of the stellar models during the TP-AGB phase, and tables of the stellar yields for 74 species from hydrogen through to sulfur, and for a small number of iron-group nuclei. All tables are available for download. Our results have many applications including use in population synthesis studies and the chemical evolution of galaxies and stellar systems, and for comparison to the composition of AGB and post-AGB stars and planetary nebulae.
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In the citing paper
“The first stellar yields for a large range of masses, and metallicities from detailed AGB models were published by Karakas & Lattanzio (2007), with an update by Karakas (2010).”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Karakas & Lattanzio 2007
In the citing paper
“During HBB the temperatures at the base of the convective envelope are higher than in the H shell during the first ascent of the giant branch, reaching T bce ≳ 100 MK in the lowest metallicity, massive AGB stars”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Karakas & Lattanzio 2007
In the citing paper
“Canonical AGB models do not produce substantial quantities of elemental O and stellar yields from such models are generally negligible, except at the lowest metallicities (e.g., at Z ≤ 10 -4 Karakas & Lattanzio 2007; Campbell & Lattanzio 2008; Karakas 2010; Cristallo et al. 2011).”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Karakas & Lattanzio 2007
In the citing paper
“The stellar models in Karakas (2010) produced between ∼ 6 to 30 times less Na compared to the stellar models in Karakas & Lattanzio (2007) as a result of using updated reaction rates.”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Karakas & Lattanzio (2007)
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Metadata
- Authors
- Karakas, A., & Lattanzio, J. C.
- Affiliations
- Mount Stromlo Observatory (AU)
- Monash University (AU)
- Corresponding author
- Karakas, Amanda
- Venue
- Publications of the Astronomical Society of Australia
- Publisher
- Cambridge University Press (CUP)
- Published
- 2007
- Volume
- 24
- Issue
- 3
- Pages
- 103-117
- ISSN
- 1323-3580 (ISSN-L)
- 1448-6083
- OpenAlex
- W2097122825
- Cited by
- 312
- References
- 51
- Citations by year
- 2026: 7 · 2025: 4 · 2024: 9 · 2023: 10 · 2022: 7 · 2021: 7 · 2020: 8 · 2019: 11 · 2018: 13 · 2017: 19 · 2016: 23 · 2015: 15 · 2014: 20 · 2013: 27 · 2012: 24
- FWCI
- 17.16
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Publications of the Astronomical Society of Australia (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Australian Research Council (DP0664105)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- asymptotic giant branch stars, stellar yields, thermally pulsing AGB, stellar nucleosynthesis, low- and intermediate-mass stars, metallicity dependence, core helium flash, stellar structure, population synthesis, chemical evolution, planetary nebulae, post-AGB stars
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