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Constraints on stellar interior physics from helioseismology

Published online by Cambridge University Press:  25 May 2016

J. Christensen-Dalsgaard
J. Christensen-Dalsgaard*
Affiliation:
Teoretisk Astrofysik Center, Danmarks Grundforskningsfond, and Institut for Fysik og Astronomi, Aarhus Universitet, DK-8000 Aarhus C, Denmark

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Traditional observations of the properties of stars generally provide tests of only the gross aspects of stellar structure and evolution. The limitation lies in the amount and precision of the available data of relevance to the structure of the stellar interior, i.e., the determination of stellar effective temperatures, surface composition, luminosities and, in a few cases, masses. Additional constraints on the observed stars, such as the common age and composition normally assumed for stars in clusters or multiple systems, clearly increase the information. However, detailed information on the physics and processes of stellar interiors requires more extensive data, with a dependence on stellar structure sufficiently simple to allow unambiguous interpretation. Such data are offered by observations of stellar pulsation frequencies: they can be observed with great accuracy and their dependence of stellar structure is generally well understood. In particular, the richness and precision of the observed frequencies of solar oscillation are now offering a detailed view on the interior properties of a star.

Type
Stellar Oscillations and Pulsations
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 285 - 292
Copyright
Copyright © Kluwer 1997 

References

Andreasen, G. K. & Petersen, J. O., 1988. Astron. Astrophys. , 192, L4 Google Scholar
Antia, H. M. & Chitre, S. M., 1995. Astrophys. J. , 442, 434 Google Scholar
Baglin, A. & Lebreton, Y., 1990. Proc. IAU Colloquium No 121, Inside the Sun , p. 437 eds Berthomieu, G. & Cribier, M., Kluwer, Dordrecht.Google Scholar
Bahcall, J. N. & Pinsonneault, M. H., 1995. Rev. Mod. Phys. , 67, 781 CrossRefGoogle Scholar
Bahcall, J. N., Pinsonneault, M. H., Basu, S. & Christensen-Dalsgaard, J., 1997. Phys. Rev. Lett. , 78, 171 Google Scholar
Basu, S. & Christensen-Dalsgaard, J., 1997. Astron. Astrophys. , submitted.Google Scholar
Basu, S. et al., 1997. Mon. Not. R. astr. Soc. , submitted.Google Scholar
Basu, S., Christensen-Dalsgaard, J., Pérez Hernández, F. & Thompson, M. J., 1996. Mon. Not. R. astr. Soc. , 280, 651 Google Scholar
Bruntt, H., 1996. , .Google Scholar
Chaboyer, B., Demarque, P., Guenther, D. B. & Pinsonneault, M. H., 1995. Astrophys. J. , 446, 435 Google Scholar
Chaplin, W. J. et al., 1996. Mon. Not. R. astr. Soc. , 282, L15 Google Scholar
Christensen-Dalsgaard, J., 1997. In Proc. 18th Texas Symposium on Relativistic Astrophysics , eds Olinto, A., Frieman, J. & Schramm, D., World Scientific Press, in press.Google Scholar
Christensen-Dalsgaard, J. & Däppen, W., 1992. Astron. Astrophys. Rev. , 4, 267 Google Scholar
Christensen-Dalsgaard, J., Däppen, W., Ajukov, S. V. et al., 1996. Science , 272, 1286 Google Scholar
Christensen-Dalsgaard, J., Däppen, W. & Lebreton, Y., 1988. Nature , 336, 634 Google Scholar
Christensen-Dalsgaard, J., Dilke, F. W. W. & Gough, D. O., 1974. Mon. Not. R. astr. Soc. , 169, 429 Google Scholar
Christensen-Dalsgaard, J., Proffitt, C. R. & Thompson, M. J., 1993. Astrophys. J. , 403, L75 CrossRefGoogle Scholar
Cox, A. N., Guzik, J. A. & Kidman, R. B., 1989. Astrophys. J. , 342, 1187 Google Scholar
Däppen, W., 1992. Proc. Workshop on Astrophysical Opacities, Revista Mexicana de Astronomia y Astrofisica , 23, eds Lynas-Gray, C., Mendoza, C. & Zeippen, C., 141 Google Scholar
Dilke, F. W. W. & Gough, D. O., 1972. Nature , 240, 262 Google Scholar
Dziembowski, W. A., Pamyatnykh, A. A. & Sienkiewicz, R., 1992. Acta Astron. , 42, 5 Google Scholar
Elliott, J. R., 1995. Mon. Not. R. astr. Soc. , 277, 1567 Google Scholar
Elliott, J. R., 1996. Mon. Not. R. astr. Soc. , 280, 1244 Google Scholar
Elliott, J. R., 1997. Astron. Astrophys. , submitted.Google Scholar
Gough, D. O. & Toomre, J., 1991. Ann. Rev. Astron. Astrophys. , 29, 627 CrossRefGoogle Scholar
Gough, D. O., Kosovichev, A. G., Toomre, J. et al., 1996. Science , 272, 1296 Google Scholar
Harvey, J. W., Hill, F., Hubbard, R. P. et al., 1996. Science , 272, 1284 Google Scholar
Huebner, W. F., Merts, A. L., Magee, N. H. & Argo, M. F., 1977. Astrophysical Opacity Library , Los Alamos Scientific Laboratory Report LA-6760-M.Google Scholar
Iglesias, C. A., Rogers, F. J. & Wilson, B. G., 1992. Astrophys. J. , 397, 717 Google Scholar
Kosovichev, A. G., 1996. Astrophys. J. , 469, L61 Google Scholar
Moskalik, P., Buchler, J. R. & Marom, A., 1992. Astrophys. J. , 385, 685 CrossRefGoogle Scholar
Rogers, F. J., Swenson, F. J. & Iglesias, C. A., 1996. Astrophys. J. , 456, 902 CrossRefGoogle Scholar
Scherrer, P. H., Bogart, R. S., Bush, R. I. et al., 1996. Solar Phys. , 162, 129 Google Scholar
Simon, N. R., 1982. Astrophys. J. , 260, L87 Google Scholar
Spiegel, E. A. & Zahn, J.-P., 1992. Astron. Astrophys. , 265, 106 Google Scholar
Thompson, M. J., Toomre, J., Anderson, E. R. et al., 1996. Science , 272, 1300 Google Scholar
Tomczyk, S. et al., 1995. Solar Phys. , 159, 1 Google Scholar
Tripathy, S. C., Basu, S. & Christensen-Dalsgaard, J., 1997. In Poster Volume; Proc. IAU Symposium No 181 , eds Schmider, F.X. & Provost, J., Nice Observatory, in press.Google Scholar
Vorontsov, S. V., Baturin, V. A. & Pamyatnykh, A. A., 1992. Mon. Not. R. astr. Soc. , 257, 32 CrossRefGoogle Scholar