The DOI matches its Crossref record; 58 of the 58 references it cites were found in a registry or an index.
Evolution of massive AGB stars: II. model properties at non-solar metallicity and the fate of Super-AGB stars
Open accessAbstract
Context.Massive AGB (hereafter super-AGB or SAGB) stars ignite carbon off-center and have initial masses ranging between , the minimum initial mass for carbon ignition, and Mmas the minimum mass for the formation of an iron core collapse supernova. In this mass interval, stars more massive than will undergo an electron capture supernova (EC-SN).
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Cites
Vetterling, W. T., Teukolsky, S. A., Press, W. H., & Flannery, B. P. (1988) · Cited by 7,701
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:2000126 · Cited by 2,553
The evolution and explosion of massive stars
Woosley, S. E., Heger, A., & Weaver, T. A. (2002) · Reviews of Modern Physics · doi:10.1103/revmodphys.74.1015 · Cited by 2,247
Vassiliadis, E., & Wood, P. R. (1993) · The Astrophysical Journal · doi:10.1086/173033 · Cited by 1,253
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 1,051
Nomoto, K. (1984) · The Astrophysical Journal · doi:10.1086/161749 · Cited by 643
Stellar evolution models for Z = 0.0001 to 0.03
Pols, O. R., Schroder, K.-P., Hurley, J. R., Tout, C. A., & Eggleton, P. P. (1998) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1998.01658.x · Cited by 581
Explosions of O-Ne-Mg cores, the Crab supernova, and subluminous type II-P supernovae
Kitaura, F. S., Janka, H.-T., & Hillebrandt, W. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20054703 · Cited by 578
The Effects of Binary Evolution on the Dynamics of Core Collapse and Neutron Star Kicks
Podsiadlowski, P., Langer, N., Poelarends, A. J. T., Rappaport, S., Heger, A., & Pfahl, E. D. (2004) · The Astrophysical Journal · doi:10.1086/421713 · Cited by 544
Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs
Jose, J., & Hernanz, M. (1998) · The Astrophysical Journal · doi:10.1086/305244 · Cited by 488
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Multiple populations in globular clusters: Lessons learned from the Milky Way globular clusters
Gratton, R. G., Carretta, E., & Bragaglia, A. (2012) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-012-0050-3 · Cited by 787
The Origin of Elements from Carbon to Uranium
Kobayashi, C., Karakas, A. I., & Lugaro, M. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abae65 · Cited by 745
Formation and dynamical evolution of multiple stellar generations in globular clusters
D'Ercole, A., Vesperini, E., D'Antona, F., McMillan, S. L. W., & Recchi, S. (2008) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2008.13915.x · Cited by 657
The Evolution of Compact Binary Star Systems
Postnov, K. A., & Yungelson, L. R. (2014) · Living Reviews in Relativity · doi:10.12942/lrr-2014-3 · Cited by 486
The evolution of isotope ratios in the Milky Way Galaxy
Kobayashi, C., Karakas, A. I., & Umeda, H. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18621.x · Cited by 401
Metadata
- Authors
- Siess, L.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2007-10-02
- Volume
- 476
- Issue
- 2
- Pages
- 893-909
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2120263023
- Cited by
- 264
- References
- 58
- FWCI
- 6.64
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Siess, L. (2007). Evolution of massive AGB stars: II. model properties at non-solar metallicity and the fate of Super-AGB stars. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20078132
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
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.
