Abstract
It is shown that the oscillatory properties of the eigenfunctions can be proved rigorously for the second order problem. Models with discontinuities in density are also considered and “discontinuity modes” are shown to exist. The distribution of amplitudes of these modes is also discussed.
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References
Coddington, E. and Levinson, N. 1955, Theory of Ordinary Differential Equations, (McGraw-Hill).
Cowling, T.C. 1941, Mon. Not. R. Astr. Soc., 101, 367.
Gabriel, M. and Scuflaire re, R. 1979, Acta Astr., 29, (in press).
Landau, L. and Lifschitz, E. 1959, Fluid Mechanics, (Pergamon Press).
Ledoux, P. and Walraven, T. 1958, “Variable Stars” in Handbuch der Physik 51, 353, (ed. Flugge; Berlin: Springer).
Osaki, Y. 1975, Publ. Astron. Soc. Japan, 27, 237.
Owen, J.W. 1957, Mon. Not. R. Astr. Soc., 167, 384.
Robe, H. 1968, Ann. Astrophys., 31, 475.
Scuflaire, R. 1974, Astron. Astrophys., 36, 107.
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© 1980 Springer-Verlag
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Gabriel, M., Scuflaire, R. (1980). Properties of nonradial stellar oscillations. In: Hill, H.A., Dziembowski, W.A. (eds) Nonradial and Nonlinear Stellar Pulsation. Lecture Notes in Physics, vol 125. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-09994-8_45
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DOI: https://doi.org/10.1007/3-540-09994-8_45
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