Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-25T05:37:50.608Z Has data issue: false hasContentIssue false
  • English
  • Français

The Sun as a fundamental calibrator of stellar evolution

Published online by Cambridge University Press:  01 October 2008

Jørgen Christensen-Dalsgaard
Jørgen Christensen-Dalsgaard*
Affiliation:
Danish Asteroseismology Centre, and Department of Physics and Astronomy, Aarhus University, DK 8000 Aarhus C, Denmark email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Sun is unique amongst stars in having a precisely determined age which does not depend on the modelling of stellar evolution. Furthermore, other global properties of the Sun are known to much higher accuracy than for any other star. Also, helioseismology has provided detailed determination of the solar internal structure and rotation. As a result, the Sun plays a central role in the development and test of stellar modelling. Here I discuss solar modelling and its application to tests of asteroseismic techniques for stellar age determination.

Keywords

Sun: evolutionSun: interiorSun: helioseismologySun: fundamental parametersstars: evolutionstars: interiorstars: oscillationsstars: fundamental parametersasteroseismology
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S258: The Ages of Stars , October 2008 , pp. 431 - 442
Copyright
Copyright © International Astronomical Union 2009

References

Ahmad, Q. R., Allen, R. C., Andersen, T. C. et al. , 2002, Phys. Rev. Lett. 89, 011301Google Scholar
Appourchaux, T., Michel, E., Auvergne, M. et al. , 2008, A&A 488, 705Google Scholar
Asplund, M. 2005, ARAA 43, 481CrossRefGoogle Scholar
Asplund, M., Grevesse, N., Sauval, A. J., Allende Prieto, C., & Kiselman, D. 2004, A&A 417, 751 (Erratum: A&A 435, 339)Google Scholar
Auwers, A. 1891, Astron. Nachr. 128, 361Google Scholar
Böhm-Vitense, E. 1958, ZfA 46, 108Google Scholar
Bahcall, J. N. & Pinsonneault, M. H. 1995, (with an appendix by G. J. Wasserburg), Rev. Mod. Phys. 67, 781Google Scholar
Bahcall, J. N. & Serenelli, A. M. 2005, ApJ 626, 530Google Scholar
Bahcall, J. N., Gonzalez-Garcia, M. C., & Peña-Garay, C. 2004, J. High Energy Phys. 08, 016Google Scholar
Bahcall, J. N., Basu, S., Pinsonneault, M., & Serenelli, A. M. 2005, ApJ 618, 1049Google Scholar
Bahcall, J. N., Serenelli, A. M., & Basu, S. 2006, ApJS 165, 400Google Scholar
Barnes, S. A. 2007, ApJ 669, 1167Google Scholar
Basu, S. & Antia, H. M. 2008, Phys. Rep. 457, 217Google Scholar
Basu, S., Christensen-Dalsgaard, J., & Thompson, M. J. 2002, in: Favata, F., Roxburgh, I. W. & Galadí-Enríquezi, D. (eds), Proc. 1st Eddington Workshop, ‘Stellar Structure and Habitable Planet Finding’, ESA SP-485 (Noordwijk, The Netherlands: ESA), p. 249Google Scholar
Bonanno, A., Schlattl, H., & Paternò, L. 2002, A&A 390, 1115Google Scholar
Brown, T. M. & Christensen-Dalsgaard, J. 1998, ApJ 500, L195Google Scholar
Chaplin, W. J., Elsworth, Y., Isaak, G. R., Miller, B. A., & New, R. 2004, MNRAS 352, 1102Google Scholar
Chaplin, W. J., Serenelli, A. M., Basu, S., Elsworth, Y., New, R., & Verner, G. A. 2007, ApJ 670, 872Google Scholar
Chaplin, W. J., Houdek, G., Appourchaux, T., Elsworth, Y., New, R., & Toutain, T. 2008a, A&A 485, 813Google Scholar
Chaplin, W. J., Appourchaux, T., Arentoft, T. et al. , 2008b, Astron. Nach. 329, 549Google Scholar
Chaplin, W. J., Appourchaux, T., Arentoft, T. et al. , 2008c, in: Gizon, L. & Roth, M. (eds), Proc. HELAS II International Conference: Helioseismology, Asteroseismology and the MHD Connections, J. Phys.: Conf. Ser. 118, 012048Google Scholar
Christensen-Dalsgaard, J. 1984, in: Mangeney, A. & Praderie, F. (eds), Space Research Prospects in Stellar Activity and Variability (Paris: Paris Observatory Press), p. 11Google Scholar
Christensen-Dalsgaard, J. 1988, in: Christensen-Dalsgaard, J. & Frandsen, S. (eds), Advances in helio- and asteroseismology, Proc. IAU Symposium No 123 (Dordrecht: Reidel), p. 295Google Scholar
Christensen-Dalsgaard, J. 2002, Rev. Mod. Phys. 74, 1073Google Scholar
Christensen-Dalsgaard, J. & Thompson, M. J. 1997, MNRAS 284, 527Google Scholar
Christensen-Dalsgaard, J., Däppen, W., & Lebreton, Y. 1988, Nature 336, 634Google Scholar
Christensen-Dalsgaard, J., Däppen, W., Ajukov, S. V., et al. 1996, Science 272, 1286Google Scholar
Christensen-Dalsgaard, J., Arentoft, T., Brown, T. M., Gilliland, R. L., Kjeldsen, H., Borucki, W. J., & Koch, D. 2007, in: Handler, G. & Houdek, G. (eds), Proc. Vienna Workshop on the Future of Asteroseismology, Comm. in Asteroseismology 150, 350Google Scholar
Christensen-Dalsgaard, J., Di Mauro, M. P., Houdek, G., & Pijpers, F. 2009, A&A, in the press [arXiv:0811.1001 [astro-ph]].Google Scholar
Cunha, M. S. & Metcalfe, T. S. 2007, ApJ 666, 413Google Scholar
Demarque, P., Guenther, D. B. & Kim, Y.-C. 1999, ApJ 517, 510Google Scholar
Dziembowski, W. A. & Goode, P. R. 1997, A&A 317, 919Google Scholar
Dziembowski, W. A., Fiorentini, G., Ricci, B., & Sienkiewicz, R. 1999, A&A 343, 990Google Scholar
Elsworth, Y., Howe, R., Isaak, G. R., McLeod, C. P., & New, R. 1990, Nature 347, 536Google Scholar
Fröhlich, C. & Lean, J. 2004, A&AR 12, 273Google Scholar
Gough, D. O. 1987, Nature 326, 257Google Scholar
Gough, D. O. 1996, Observatory 116, 313Google Scholar
Gough, D. O. 2001, in: Hippel, T. von, Simpson, C. & Manset, N. (eds), Astrophysical Ages and Time Scales, ASP Conf. Ser. 245 (San Francisco: ASP), p. 31Google Scholar
Gough, D. O. 2002, in: Favata, F., Roxburgh, I. W. & Galadí-Enríquezi, D. (eds), Proc. 1st Eddington Workshop: ‘Stellar structure and habitable planet finding’, ESA SP-485 (Noordwijk, The Netherlands: ESA), p. 65Google Scholar
Gough, D. O. & Kosovichev, A. G. 1993, in: Brown, T. M. (ed.), Proc. GONG 1992: Seismic investigation of the Sun and stars, ASP Conf. Ser. 42, (San Francisco: ASP), p. 351Google Scholar
Gough, D. O. & Novotny, E. 1990, Solar Phys. 128, 143Google Scholar
Gough, D. O. & Weiss, N. O. 1976, MNRAS 176, 589Google Scholar
Grevesse, N. & Noels, A. 1993, in: Prantzos, N., Vangioni-Flam, E. & Cassé, M. (eds), Origin and evolution of the Elements, (Cambridge: Cambridge Univ. Press), p. 15Google Scholar
Grundahl, F., Arentoft, T., Christensen-Dalsgaard, J., Frandsen, S., Kjeldsen, H., & Rasmussen, P. K. 2008, in: Gizon, L. & Roth, M. (eds), Proc. HELAS II International Conference: Helioseismology, Asteroseismology and the MHD Connections, J. Phys.: Conf. Ser. 118, 012041Google Scholar
Guenther, D. B. & Demarque, P. 1997, ApJ 484, 937Google Scholar
Guzik, J. A. 2006, in: Fletcher, K. (ed.), Proc. SOHO 18/GONG 2006/HELAS I Conf. Beyond the spherical Sun, ESA SP-624, (Noordwijk, The Netherlands: ESA).Google Scholar
Guzik, J. A. 2008, MemSAI 79, 481Google Scholar
Haxton, W. C. 2008, PASA 25, 44Google Scholar
Haxton, W. C., Parker, P. D., & Rolfs, C. E. 2006, Nucl. Phys. A. 777, 226Google Scholar
Houdek, G. & Gough, D. O. 2007a, MNRAS 375, 861Google Scholar
Houdek, G. & Gough, D. O. 2007b, in: Stancliffe, R. J., Dewi, J., Houdek, G., Martin, R. G. & Tout, C. A (eds), Unsolved Problems in Stellar Physics, AIP Conf. Proc. 948 (Melville: AIP), p. 219Google Scholar
Houdek, G. & Gough, D. O. 2008, in: Deng, L. & Chan, K. L. (eds), The Art of Modelling Stars in the 21st Century, Proc. IAU Symposium No 252 (Cambridge: Cambridge University Press), p. 149Google Scholar
Howe, R., Komm, R. W., & Hill, F. 2002, ApJ 580, 1172Google Scholar
Iglesias, C. A. & Rogers, F. J. 1996, ApJ 464, 943Google Scholar
Kjeldsen, H., Bedding, T. R., & Christensen-Dalsgaard, J. 2008a, ApJ 683, L175Google Scholar
Kjeldsen, H., Bedding, T. R., & Christensen-Dalsgaard, J. 2008b, in: Pont, F., Queloz, D. & Sasselov, D. D. (eds), Transiting Planets, Proc. IAU Symposium No 253 (Cambridge: Cambridge University Press), in the press [arXiv:0807.0508v1 [astro-ph]]Google Scholar
Ludwig, H.-G., Freytag, B., & Steffen, M. 1997, in: Pijpers, F. P., Christensen-Dalsgaard, J. & Rosenthal, C. S., , C. S. (eds), SCORe’96: Solar Convection and Oscillations and their Relationship, (Dordrecht: Kluwer), p. 59CrossRefGoogle Scholar
Ludwig, H.-G., Freytag, B., & Steffen, M. 1999, A&A 346, 111Google Scholar
Mazumdar, A., Basu, S., Collier, B. L., & Demarque, P. 2006, MNRAS 372, 949Google Scholar
Monteiro, M. J. P. F. G., Christensen-Dalsgaard, J., & Thompson, M. J. 2002, in: Favata, F., Roxburgh, I. W. & Galadí-Enríquezi, D. (eds), Proc. 1st Eddington Workshop: ‘Stellar structure and habitable planet finding’, ESA SP-485 (Noordwijk, The Netherlands: ESA), p. 291Google Scholar
Mosser, B., Appourchaux, T., Catala, C., Buey, J.-T. and the SIAMOIS team 2008, in: Gizon, L. & Roth, M. (eds), Proc. HELAS II International Conference: Helioseismology, Asteroseismology and the MHD Connections, J. Phys.: Conf. Ser. 118, 012042Google Scholar
Otí Floranes, H., Christensen-Dalsgaard, J., & Thompson, M. J. 2005, MNRAS 356, 671Google Scholar
Robertson, R. G. H. 2006, Prog. Particle Nuclear Phys. 57, 90Google Scholar
Rogers, F. J. & Nayfonov, A. 2002, ApJ 576, 1064Google Scholar
Rosenthal, C. S., Christensen-Dalsgaard, J., & Nordlund, Å., Stein, R. F. & Trampedach, R. 1999, A&A 351, 689Google Scholar
Roxburgh, I. W. & Vorontsov, S. V. 2003, A&A 411, 215Google Scholar
Roxburgh, I. W. 2002, in: Favata, F., Roxburgh, I. W. & Galadí-Enríquezi, D. (eds), Proc. 1st Eddington Workshop: ‘Stellar structure and habitable planet finding’, ESA SP-485 (Noordwijk, The Netherlands: ESA), p. 75Google Scholar
Sackmann, I.-Juliana & Boothroyd, A. I. 2003, ApJ 583, 1024Google Scholar
Thompson, M. J., Christensen-Dalsgaard, J., Miesch, M. S., & Toomre, J. 2003, ARAA 41, 599CrossRefGoogle Scholar
Toutain, T. & Kosovichev, A. G. 2005, ApJ 622, 1314Google Scholar
Trampedach, R., Stein, R. F., Christensen-Dalsgaard, J., & Nordlund, A&A. 1999, in: Giménez, A., Guinan, E.F. & Montesinos, B. (eds), Theory and Tests of Convection in Stellar Structure, ASP Conf. Ser. 173 (San Francisco: ASP), p. 233Google Scholar
Ulrich, R. K. 1986, ApJ 306, L37Google Scholar