The DOI matches its Crossref record; 69 of the 69 references it cites were found in a registry or an index.
Grids of stellar models with rotation: II. WR populations and supernovae/GRB progenitors at Z= 0.014
Open accessAbstract
Context. In recent years, many very interesting observations have appeared concerning the positions of Wolf-Rayet (WR) stars in the Hertzsprung-Russell diagram (HRD), the number ratios of WR stars, the nature of Type Ibc supernova (SN) progenitors, long and soft gamma ray bursts (LGRB), and the frequency of these various types of explosive events. These observations represent key constraints on massive star evolution.
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Citations
Cites
The Luminosity Function and Stellar Evolution.
Salpeter, E. E. (1955) · The Astrophysical Journal · doi:10.1086/145971 · Cited by 8,697
Gamma-ray bursts from stellar mass accretion disks around black holes
Woosley, S. E. (1993) · The Astrophysical Journal · doi:10.1086/172359 · Cited by 2,554
How Massive Single Stars End Their Life
Heger, A., Fryer, C. L., Woosley, S. E., Langer, N., & Hartmann, D. H. (2003) · The Astrophysical Journal · doi:10.1086/375341 · Cited by 2,165
An unusual supernova in the error box of the γ-ray burst of 25 April 1998
Galama, T. J., Vreeswijk, P. M., van Paradijs, J., Kouveliotou, C., Augusteijn, T., Böhnhardt, H., Brewer, J. P., Doublier, V., Gonzalez, J.-F., Leibundgut, B., et al. (1998) · Nature · doi:10.1038/27150 · Cited by 1,921
The Supernova–Gamma-Ray Burst Connection
Woosley, S. E., & Bloom, J. S. (2006) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.072103.150558 · Cited by 1,766
Mass-loss predictions for O and B stars as a function of metallicity
Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20010127 · Cited by 1,727
Grids of stellar models with rotation: I. Models from 0.8 to 120 M⊙at solar metallicity (Z= 0.014)⋆
Ekström, S., Georgy, C., Eggenberger, P., Meynet, G., Mowlavi, N., Wyttenbach, A., Granada, A., Decressin, T., Hirschi, R., Frischknecht, U., et al. (2012) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201117751 · Cited by 1,712
Self-citationNeutron Star Structure and the Equation of State
Lattimer, J. M., & Prakash, M. (2001) · The Astrophysical Journal · doi:10.1086/319702 · Cited by 1,665
Progenitors of Core-Collapse Supernovae
Smartt, S. J. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101737 · Cited by 1,231
Physical Properties of Wolf-Rayet Stars
Crowther, P. A. (2007) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.45.051806.110615 · Cited by 990
Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Choi, J., Dotter, A., Conroy, C., Cantiello, M., Paxton, B., & Johnson, B. D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/102 · Cited by 2,922
Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
Smith, N. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040025 · Cited by 1,042
“Standard single-star models predict MWR ≃ 35M⊙ at Z⊙ (Georgy et al. 2012, Heger et al. 2003), in- 26 Smith creasing to about 45 and 70M⊙ at ZLMC and ZSMC , respectively (Heger et al. 2003).”
BackgroundPREPARING FOR AN EXPLOSION: HYDRODYNAMIC INSTABILITIES AND TURBULENCE IN PRESUPERNOVAE
Smith, N., & Arnett, W. D. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/785/2/82 · Cited by 253
Number of stars in the Sun’s birth cluster revisited
Arakawa, S., & Kokubo, E. (2023) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202244743 · Cited by 18
Metadata
- Authors
- Georgy, C., Ekström, S., Meynet, G., Massey, P., Levesque, E. M., Hirschi, R., Eggenberger, P., & Maeder, A.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-05-30
- Volume
- 542
- Pages
- A29
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4297902381
- Cited by
- 269
- References
- 69
- FWCI
- 13.82
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: Grids of stellar models with rotation: II. WR populations and supernovae/GRB progenitors at Z= 0.014. https://app.cochat.ai/papers/10.1051/0004-6361/201118340
- The paper
- Georgy, C., Ekström, S., Meynet, G., Massey, P., Levesque, E. M., Hirschi, R., Eggenberger, P., & Maeder, A. (2012). Grids of stellar models with rotation: II. WR populations and supernovae/GRB progenitors at Z= 0.014. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201118340
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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