The DOI matches its Crossref record; 51 of the 51 references it cites were found in a registry or an index.
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.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
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)
Citations
Cites
Abundances of the elements: Meteoritic and solar
Anders, E., & Grevesse, N. (1989) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(89)90286-x · Cited by 8,722
The distribution of low-mass stars in the Galactic disc
Kroupa, P., Tout, C., & Gilmore, G. (1993) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/262.3.545 · Cited by 1,347
Vassiliadis, E., & Wood, P. R. (1993) · The Astrophysical Journal · doi:10.1086/173033 · Cited by 1,253
The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy
Beers, T. C., & Christlieb, N. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134057 · Cited by 1,223
Busso, M., Roberto Gallino, A., & Wasserburg, G. J. (1999) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.37.1.239 · Cited by 1,144
Evolution of Asymptotic Giant Branch Stars
Herwig, F. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.072103.150600 · Cited by 1,062
Abundance Variations within Globular Clusters
Gratton, R., Sneden, C., & Carretta, E. (2004) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.133945 · Cited by 885
Abundances of the heavy elements in the Magellanic Clouds. III - Interpretation of results
Russell, S. C., & Dopita, M. A. (1992) · The Astrophysical Journal · doi:10.1086/170893 · Cited by 630
Winckel, H. V. (2003) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.41.071601.170018 · Cited by 453
A new synthetic model for asymptotic giant branch stars
Izzard, R. G., Tout, C. A., Karakas, A. I., & Pols, O. R. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07446.x · Cited by 304
Self-citation
Research works printed but not linked: 34
- Stancliffe, 2004, MmSAI, 75, 670
- Siess, 2006, AandA, 448, 717
- Marigo, 2001, AandA, 370, 194
- Izzard, 2006, AandA, 460, 565
- Karakas A. I. , 2003, PhD thesis, Monash University
- Thielemann, 1986, Advances in Nuclear Astrophysics, 525
- Campbell S. W. , 2007, PhD thesis, Monash University
- Frost, 1998, AandA, 332, L17
- Forestini, 1997, AandAS, 123, 241
- Wagenhuber, 1998, AandA, 340, 183
- Ventura, 2005, AandA, 431, 279
- Asplund, 2005, in ASPC 336: Cosmic Abundances as Records of Stellar Evolution and Nucleo-synthesis, 25
- Lugaro, 2007, AandA, 461, 657
- Ventura, 2002, AandA, 393, 215
- Palacios, 2006, AandA, 453, 261
- Ventura, 2005, AandA, 439, 1075
- Izzard, 2007, AandA, 466, 641
- Blöcker, 1991, AandA, 244, L43
- Groenewegen, 1993, AandA, 267, 410
- Lattanzio, 1996, MmSAI, 67, 729
- Marigo, 1996, AandA, 313, 545
- Goriely, 2000, AandA, 362, 599
- Garcia-Hernandez, 2007, AandA, 462, 711
- Renzini, 1981, AandA, 94, 175
- McSaveney J. A. , Wood P. R. , Scholz M. , Lattanzio J. C. & Hinkle K. H. , 2007, MNRAS, in press
- Jorissen, 1992, AandA, 261, 164
- van den Hoek, 1997, AandAS, 123, 305
- Charbonnel, 1994, AandA, 282, 811
- Mowlavi, 1999, AandA, 344, 617
- Guandalini, 2006, AandA, 445, 1069
- Blöcker, 1995, AandA, 297, 727
- Sterling N. C. & Dinerstein H. L. , 2007, ApJS, in press
- Yong, 2003, AandA, 402, 985
- Charbonnel, 2007, AandA, 467, L15
Cited by
Sorted by citations
Zwart, S. P., McMillan, S. L. W., & Gieles, M. (2010) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081309-130834 · Cited by 1,265
The Origin of Elements from Carbon to Uranium
Kobayashi, C., Karakas, A. I., & Lugaro, M. A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abae65 · Cited by 831
Self-citationUpdated stellar yields from asymptotic giant branch models
Karakas, A. I. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.16198.x · Cited by 758
Self-citationMultiple Stellar Populations in Globular Clusters
Bastian, N., & Lardo, C. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051839 · Cited by 737
Jermyn, A. S., Bauer, E. B., Schwab, J., Farmer, R., Ball, W. H., Bellinger, E. P., Dotter, A., Joyce, M., Marchant, P., Mombarg, J. S. G., et al. (2023) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/acae8d · Cited by 736
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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
