Astrophysics: Influence of gravity waves on the internal rotation and Li abundance of solar-type stars

Science

Volumn 309, Issue 5744, 2005, Pages 2189-2191

  Charbonnel, Corinne ^a,b   Talon, Suzanne ^c  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b OBSERVATOIRE MIDI PYRÉNÉES   (France)

^c UNIVERSITÉ DE MONTRÉAL   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

ANGLE MEASUREMENT; HYDRODYNAMICS; MATHEMATICAL MODELS;

HYDRODYNAMIC MODELS; SOLAR-TYPE STARS;

LITHIUM;

LITHIUM;

ASTROPHYSICS;

ANGULAR MOMENTUM; ARTICLE; ASTRONOMY; EVOLUTION; GRAVITY; HYDRODYNAMICS; MODEL; OSCILLATION; PHYSICAL PHENOMENA; PRIORITY JOURNAL; ROTATION; SOLAR TYPE STAR; SUN; THERMODYNAMICS;

EID: 25844529343     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1116849     Document Type: Article

References (33)

1. W. J. Chaplin et al., Mon. Not. R. Astron. Soc. 308, 405 (1999).
2. S. Couvidat et al., Astrophys. J. 597, L77 (2003).
3. B. Chaboyer, P. Demarque, M. H. Pinsonneault, Astrophys. J. 441, 865 (1995).
4. J. Matias, J.-P. Zahn, in Sounding Solar and Stellar Interiors, J. Provost, F.-X. Schmider, Eds. (IAU Symposium 181, Observatoire de la Côte d'Azur, Nice, France, 1998), pp. 103-104.
5. A. Maeder, C. Meynet, Annu. Rev. Astron. Astrophys. 38, 143 (2000).
6. P. Charbonneau, K. B. MacCregor, Astrophys. J. 417, 762 (1993).
7. P. Eggenberger, A. Maeder, G. Meynet, Astron. Astrophys. 440, L9 (2005).
8. J.-P. Zahn, S. Talon, J. Matias, Astron. Astrophys. 322, 320 (1997).
9. P. Kumar, E. Quataert, Astrophys. J. 475, L143 (1997).
10. M. E. McIntyre, in Perspectives in Fluid Dynamics: A Collective Introduction to Current Research, G. K. Batchetor, H. K. Moffatt, M. C. Worster, Eds. (Cambridge Univ. Press, Cambridge, 2003), pp. 557-624.
11. M. P. Baldwin et al., Rev. Geophys. 39, 179 (2001).
12. O. Ringot, Astron. Astrophys. 335, L89 (1998).
13. P. Kumar, S. Talon, J.-P. Zahn, Astrophys. J. 520, 859 (1999).
14. S. Talon, P. Kumar, J.-P. Zahn, Astrophys. J. 574, L175 (2002).
15. S. Talon, C. Charbonnel, Astron. Astrophys., Astron. Astrophys. 440, 981 (2005).
16. c = 1/4, Ω is the rotation rate, r is the radial coordinate, K is the thermal diffusivity, g is the gravitational acceleration, and θ is the potential temperature.
17. S. D. Kawaler, Astrophys. J. 333, 236 (1988).
18. Y. Gaigé, Astron. Astrophys. 269, 267 (1993).
19. P. Goldreich, N. Murray, P. Kumar, Astrophys. J. 424, 466 (1994).
20. L ≈ L/v is the convective time.
21. N. E. Hurlburt, J. Toomre, J. M. Massaguer, Astrophys. J. 311, 563 (1986).
22. B. Dintrans, A. Brandenburg, A. Nordlund, R. F. Stein, Astron. Astrophys. 438, 365 (2005).
23. G. Barnes, K. B. MacGregor, P. Charbonneau, Astrophys. J. 498, L169 (1998).
24. D. Gough, M. E. McIntyre, Nature 394, 755 (1998).
25. G. Barnes, P. Charbonneau, K. B. MacGregor, Astrophys. J. 511, 466 (1999).
26. S. Balachandran, Astrophys. J. 446, 203 (1995).
27. B. F. Jones, D. Fischer, D. R. Soderblom, Astron. J. 117, 330 (1999).
28. L. Pasquini et al., Astron. Astrophys. 424, 951 (2004).
29. S. Randich, L. Pasquini, R. Pallavicini, Astron. Astrophys. 356, L25 (2000).
30. P. Sestito, S. Randich, R. Pallavicini, Astron. Astrophys. 426, 809 (2000).
31. D. R. Soderblom, S. B. Fedele, B. F. Jones, J. R. Stauffer, C. F. Prosser, Astron. J. 106, 1080 (1993).
32. J. A. Thorburn, L. M. Hobbs, C. P. Detiyannis, M. H. Pinsonneault, Astrophys. J. 415, 150 (1993).
33. We thank J.-O. Goussard, M. Grenon, G. Meynet, D. Pfenniger, and D. Schaerer, as well as anonymous referees and our editor for suggestions that improved the clarity of this text Supported by the Natural Sciences and Engineering Research Council of Canada (ST.).