The DOI matches its Crossref record; 19 of the 19 references it cites were found in a registry or an index.
Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars
Open accessAbstract
The Sun's rotation profile and lithium content have been difficult to understand in the context of conventional models of stellar evolution. Classical hydrodynamic models predict that the solar interior must rotate highly differentially, in disagreement with observations. It has recently been shown that internal waves produced by convection in solar-type stars produce an asymmetric, shear layer oscillation, similar to Earth's quasi-biennial oscillation, that leads to efficient angular momentum redistribution from the core to the envelope. We present results of a model that successfully reproduces both the rotation profile and the surface abundance of lithium in solar-type stars of various ages.
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Cites
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Baldwin, M. P., Gray, L. J., Dunkerton, T. J., Hamilton, K., Haynes, P. H., Randel, W. J., Holton, J. R., Alexander, M. J., Hirota, I., Horinouchi, T., et al. (2001) · Reviews of Geophysics · doi:10.1029/1999rg000073 · Cited by 2,113
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
Angular momentum loss in low-mass stars
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Inevitability of a magnetic field in the Sun's radiative interior
Gough, D. O., & McIntyre, M. E. (1998) · Nature · doi:10.1038/29472 · Cited by 374
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Talon, S., & Charbonnel, C. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20053020 · Cited by 211
Self-citationStellar evolution with rotation and magnetic fields: IV. The solar rotation profile
Eggenberger, P., Maeder, A., & Meynet, G. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:200500156 · Cited by 189
Angular Momentum Transport in Magnetized Stellar Radiative Zones. II. The Solar Spin-down
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The Lithium Dip in M67: Comparison with the Hyades, Praesepe, and NGC 752 Clusters
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Cited by
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
“The solar Li depletion cannot be explained by standard models based on the mixing length theory of convection but requires additional mixing below the convection zone (Brun, Turck-Chièze & Zahn 1999; Charbonnel & Talon 2005).”
BackgroundMESA 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
Asteroseismology of Solar-Type and Red-Giant Stars
Chaplin, W. J., & Miglio, A. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-140938 · Cited by 527
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
- Charbonnel, C., & Talon, S.
- Venue
- Science
- Published
- 2005-09-30
- Volume
- 309
- Issue
- 5744
- Pages
- 2189-2191
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2052297777
- Cited by
- 377
- References
- 19
- FWCI
- 11.91
- Type
- journal article
- Language
- en
- Open access
- green
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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.
