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Excitation and damping of solar and stellar oscillations

Published online by Cambridge University Press:  03 August 2017

S.M. Chitre
S.M. Chitre*
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay - 400005, India

Abstract

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Variable stars can be broadly classified into two categories: (a) High amplitude pulsators like Cepheids and RR Lyrae variables, (b) Low amplitude pulsators like Sun and Sun-like stars. The study of stellar pulsations has opened the possibility of using the oscillatory modes to probe the internal structure and dynamics of these stars. The cause of pulsational instability for a majority of stars is the partial ionisation of the abundant elements present in the envelope of the stars, while some instabilities are driven by the transfer of momentum from the medium to the oscillating elements. Various mechanisms responsible for exciting and limiting the solar and stellar oscillations are discussed.

Type
Chapter 6: Excitation and Damping of Solar and Stellar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 345 - 357
Copyright
Copyright © Reidel 1988 

References

Ando, H. and Osaki, Y., 1975, Publ. Astron. Soc. Japan, 27, 581.Google Scholar
Antia, H.M., Chitre, S.M. and Narasimha, D., 1982, Solar Phys., 77, 303.Google Scholar
Antia, H.M., Chitre, S.M. and Gough, D.O., 1986. These Proceedings.Google Scholar
Baker, N. and Gough, D.O., 1979, Astrophys. J., 234, 232.Google Scholar
Berthomeiu, G., Cooper, A.J., Gough, D.O., Osaki, Y., Provost, J. and Rocca, A., 1979, ‘Nonradial and Nonlinear Stellar Pulsation’ (ed. Hill, H.A. and Dziembowski, W.A.: Springer, Berlin).Google Scholar
Blackwell, D.E. and Shallis, M.J., 1977, Mon. Not. Roy. Astron. Soc., 180, 177.Google Scholar
Brickhill, A.J., 1975, Mon. Not. Roy. Astron. Soc., 170, 404.Google Scholar
Chanmugam, G., 1972, Nature Phys. Sci., 236, 83.Google Scholar
Christensen-Dalsgaard, J., 1982, Mon. Not. Roy. Astron. Soc., 199, 735.Google Scholar
Christensen-Dalsgaard, J. and Frandsen, S., 1983, Solar Phys., 82, 469.Google Scholar
Claverie, A., Isaak, G.R., McLeod, C.P., van der Raay, H.B. and Roca Cortes, T., 1979, Nature, 282, 591.Google Scholar
Cox, A.N., Starrfield, S.G., Kidman, R.B. and Pesnell, W.D., 1986 (Los Alamos National Laboratory Preprint).Google Scholar
Cox, J.P., 1976, Proc. Solar and Stellar Pulsation Conf. (ed. Cox, A.N. and Deupree, R.G., Los Alomos Publ.)Google Scholar
Cox, J.P., 1980, ‘Theory of Stellar Pulsation’ (Princeton Univ. Press, Princeton).Google Scholar
Deubner, F.-L., 1975, Astron. Astrophys., 44, 371.Google Scholar
Deupree, R.G., 1977a, Astrophys. J., 211, 509.Google Scholar
Deupree, R.G., 1977b, Astrophys. J., 215, 232.Google Scholar
Dolez, N. and Gough, D.O., 1982, ‘Pulsations in Classical and Cataclysmic Variable Stars’ (ed. Cox, J.P. and Hansen, C.J., JILA, Boulder).Google Scholar
Duvall, T.L. Jr. and Harvey, J.W., 1983, Nature, 302, 24.Google Scholar
Dziembowski, W.A., 1979, ‘Nonradial and Nonlinear Stellar Pulsation’ (ed. Hill, H.A. and Dziembowski, W.A.: Spinger, Berlin).Google Scholar
Dziembowski, W.A., 1984, ‘Theoretical Problems in Stellar Stability and Oscillations’ (Proc 25th Liege Colloquium, ed. Gabriel, M. and Noels, A.).Google Scholar
Dziembowski, W.A. and Goode, P.R., 1985. Preprint. Google Scholar
Fossat, E., Grec, G., Gelly, B. and Decanini, Y., 1984, Comptes Rendus Acad. Sci. Paris, Ser II, 299, 17.Google Scholar
Fossat, E., Gelly, B. and Grec, G., 1986, ‘Seismology of the Sun and the Distant Stars’ (ed. Gough, D.O., D. Reidel: Dordrecht).Google Scholar
Goldreich, P. and Keeley, D.A., 1977, Astrophys. J., 211, 934.Google Scholar
Gonczi, G. and Osaki, Y., 1980, Astron. Astrophys., 84, 304.Google Scholar
Gonczi, G., 1981, Astron. Astrophys., 96, 138.Google Scholar
Grec, G., Fossat, E. and Pomerantz, M., 1983, Solar Phys., 82, 55.Google Scholar
Isaak, G.R., 1986, ‘Seismology of the Sun and the Distant Stars’ (ed. Gough, D.O., D. Reidel: Dordrecht).Google Scholar
Kidman, R.B. and Cox, A.N., 1984, ‘Solar Seismology from Space’ (JPL Publication).Google Scholar
Kurtz, D.W., 1982, Mon. Not. Roy. Astron. Soc., 200, 807.Google Scholar
Kurtz, D.W. and Seeman, J., 1983, Mon. Not. Roy. Astron. Soc., 205, 11.Google Scholar
Lacy, C.H., 1977, Astrophys. J. Suppl., 34, 479.Google Scholar
Leighton, R.B., Noyes, R.W. and Simon, G.W., 1962, Astrophys. J., 135, 474.Google Scholar
Noyes, R.W., Baliunas, S.L., Belserene, E., Duncan, D.K., Horne, J. and Widrow, L., 1984, Astrophys. J., 285, L23.Google Scholar
Osaki, Y. and Hansen, C.J., 1973, Astrophys. J., 185, 277.Google Scholar
Osaki, Y., 1974, Astrophys. J., 189, 469.Google Scholar
Papaloizous, J. and Pringle, J.E., 1978, Mon. Not. Roy. Astron. Soc., 182, 423.Google Scholar
Shibahashi, H., 1983, Astrophys. J., 275, L5.Google Scholar
Stellingwerf, R.F., 1979, Astrophys. J., 227, 935.Google Scholar
Ulrich, R.K. and Rhodes, E.J. Jr., 1977, Astrophys. J., 218, 521.Google Scholar
Unno, W., 1976, ‘Problems of Stellar Convection’ (IAU Colloquium 38 ed. Spiegel, E.A. and Zahn, J.P., Springer: Berlin).Google Scholar
Unno, W., Osaki, Y., Ando, H. and Shibahashi, H., 1979, ‘Nonradial Oscillations of Stars’ (University of Tokyo Press, Tokyo).Google Scholar
Warner, B. and Robinson, E.L., 1972, Nature, Phys. Sci., 234, 2.Google Scholar
Winget, D.E., Van Horn, H.M. and Hansen, C.J., 1981, Astrophys. J., 245, 633.Google Scholar
Winget, D.E., These Proceedings.Google Scholar