The DOI matches its Crossref record; 74 of the 74 references it cites were found in a registry or an index.
Thermohaline instability and rotation-induced mixing: III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities⋆
Open accessAbstract
Context. The availability of asteroseismic constraints for a large sample of stars from the missions CoRoT and Kepler paves the way for various statistical studies of the seismic properties of stellar populations.
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Citations
Cites
The Chemical Composition of the Sun
Asplund, M., Grevesse, N., Sauval, A. J., & Scott, P. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.46.060407.145222 · Cited by 9,346
Iglesias, C. A., & Rogers, F. J. (1996) · The Astrophysical Journal · doi:10.1086/177381 · Cited by 3,020
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-citationThermonuclear reaction rates V
Caughlan, G. R., & Fowler, W. A. (1988) · Atomic Data and Nuclear Data Tables · doi:10.1016/0092-640x(88)90009-5 · Cited by 1,465
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
Vassiliadis, E., & Wood, P. R. (1993) · The Astrophysical Journal · doi:10.1086/173033 · Cited by 1,253
Rotating massive main-sequence stars: I. Grids of evolutionary models and isochrones⋆
Brott, I., de Mink, S. E., Cantiello, M., Langer, N., de Koter, A., Evans, C. J., Hunter, I., Trundle, C., & Vink, J. S. (2011) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201016113 · Cited by 890
The Evolution of Rotating Stars
Maeder, A., & Meynet, G. (2000) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.38.1.143 · Cited by 844
Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
Bedding, T. R., Mosser, B., Huber, D., Montalbán, J., Beck, P., Christensen-Dalsgaard, J., Elsworth, Y. P., García, R. A., Miglio, A., Stello, D., et al. (2011) · Nature · doi:10.1038/nature09935 · Cited by 608
Detection of possible p-mode oscillations on Procyon
Brown, T. M., Gilliland, R. L., Noyes, R. W., & Ramsey, L. W. (1991) · The Astrophysical Journal · doi:10.1086/169725 · Cited by 605
Cited by
Spin down of the core rotation in red giants
Mosser, B., Goupil, M. J., Belkacem, K., Marques, J. P., Beck, P. G., Bloemen, S., De Ridder, J., Barban, C., Deheuvels, S., Elsworth, Y., et al. (2012) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201220106 · Cited by 462
Improved angular momentum evolution model for solar-like stars
Gallet, F., & Bouvier, J. (2013) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201321302 · Cited by 373
Metadata
- Authors
- Lagarde, N., Decressin, T., Charbonnel, C., Eggenberger, P., Ekström, S., & Palacios, A.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2012-07
- Volume
- 543
- Pages
- A108
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4292399191
- Cited by
- 283
- References
- 74
- FWCI
- 11.16
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: Thermohaline instability and rotation-induced mixing: III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities⋆. https://app.cochat.ai/papers/10.1051/0004-6361/201118331
- The paper
- Lagarde, N., Decressin, T., Charbonnel, C., Eggenberger, P., Ekström, S., & Palacios, A. (2012). Thermohaline instability and rotation-induced mixing: III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities⋆. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201118331
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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.
