The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Grids of stellar models with rotation: I. Models from 0.8 to 120 M⊙at solar metallicity (Z= 0.014)⋆
Open accessAbstract
Aims. Many topical astrophysical research areas, such as the properties of planet host stars, the nature of the progenitors of different types of supernovae and gamma ray bursts, and the evolution of galaxies, require complete and homogeneous sets of stellar models at different metallicities in order to be studied during the whole of cosmic history. We present here a first set of models for solar metallicity, where the effects of rotation are accounted for in a homogeneous way.
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Cites
Ferguson, J. W., Alexander, D. R., Allard, F., Barman, T., Bodnarik, J. G., Hauschildt, P. H., Heffner‐Wong, A., & Tamanai, A. (2005) · The Astrophysical Journal · doi:10.1086/428642 · Cited by 1,327
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
“This is for physical parameters from model ZAMS stars from Ekström et al. (2012); note that the Vink et al. recipe depends on L, eff , M , and v∞, whereas the de Jager prescription uses only L and Teff .”
BackgroundMethodde Mink, S. E., Langer, N., Izzard, R. G., Sana, H., & de Koter, A. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/764/2/166 · Cited by 573
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
Pecaut, M. J., & Mamajek, E. E. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1300 · Cited by 407
Metadata
- Authors
- Ekström, S., Georgy, C., Eggenberger, P., Meynet, G., Mowlavi, N., Wyttenbach, A., Granada, A., Decressin, T., Hirschi, R., Frischknecht, U., Charbonnel, C., & Maeder, A.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-01
- Volume
- 537
- Pages
- A146
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4292508300
- Cited by
- 1,712
- References
- 1
- FWCI
- 44.07
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: Grids of stellar models with rotation: I. Models from 0.8 to 120 M⊙at solar metallicity (Z= 0.014)⋆. https://app.cochat.ai/papers/10.1051/0004-6361/201117751
- The paper
- Ekström, S., Georgy, C., Eggenberger, P., Meynet, G., Mowlavi, N., Wyttenbach, A., Granada, A., Decressin, T., Hirschi, R., Frischknecht, U., Charbonnel, C., & Maeder, A. (2012). Grids of stellar models with rotation: I. Models from 0.8 to 120 M⊙at solar metallicity (Z= 0.014)⋆. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201117751
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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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