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Accretion Disc Instabilities

Published online by Cambridge University Press:  07 August 2017

A.R. King
A.R. King*
Affiliation:
Astronomy Group University of Leicester Leicester LE1 7RH, U.K.

Abstract

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I give a brief discussion of accretion disc instabilities, concentrating mainly on tidal instabilities caused by the presence of a binary companion. The superhumps observed in superoutbursts of SU UMa dwarf novae probably result from the excitation of a resonance in the accretion disc near the 3:1 commensurability with the binary orbit. This resonance can only appear for mass ratios q = M2/M1 < qerit ≃ 0.25 – 0.33: for larger mass ratios the available resonances are considerably weaker. Application of this picture to other types of binary suggests that the condition q < qerit may be necessary but not sufficient. Further, some cataclysmic systems show phenomena which could be tidal in origin even though the condition evidently fails.

Type
Invited Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 195 - 203
Copyright
Copyright © Kluwer 1992 

References

Bailey, J., 1990 Mon. Not. R. astr. Soc. 243, 57.Google Scholar
Bailyn, C.D., 1991, Yale University preprint.Google Scholar
Bath, G.T. and Pringle, J.E., 1981, Mon. Not. R. astr. Soc. 194, 967.Google Scholar
Bath, G.T. and Pringle, J.E., 1982, Mon. Not. R. astr. Soc. 199, 267 Google Scholar
Eggleton, P. P., 1983, Astrophys. J. 268, 368.Google Scholar
Ferrario, L., Wickramasinghe, D.T. and King, A.R., 1991, preprint Google Scholar
Frank, J., King, A.R., and Raine, D.J., 1992, Accretion Power in Astrophysics , 2nd Ed., Cambridge University Press.Google Scholar
King, A. R., 1988, Quart. J. R. astr. Soc. 29, 1.Google Scholar
Hameury, J.M., King, A.R., and Lasota, J.P., 1990 Astrophys. J. 353, 585.Google Scholar
Hénon, M., 1965, Ann. d'Astr. 28, 992.Google Scholar
Lubow, S.H., 1991a, Astrophys. J. 381, to appear.Google Scholar
Lubow, S.H., 1991b, Astrophys. J. 381, to appear.Google Scholar
Meyer, F. and Meyer-Hofmeister, E., 1981, Astr. Astrophys. 104 L10.Google Scholar
McClintock, J.E. and Remillard, R.A., 1986, Astrophys. J. 308, 110.Google Scholar
McClintock, J.E. and Remillard, R.A., 1990, Astrophys. J. 350, 386.Google Scholar
Rosen, S.R., Mason, K.O., and Córdova, F.A., 1988, Mon. Not. R. astr. Soc 231, 549.Google Scholar
Ricketts, M.J., King, A.R. and Raine, D.J., 1979 Mon. Not. R. astr. Soc. 186, 233.Google Scholar
Ritter, H., 1990, Astr. Astrophys Supp. 85, 1179.Google Scholar
Shafter, A.W., Robinson, E.L., Crampton, D., Warner, B. and Prestage, R.M., 1990, in Accretion-Powered Compact Binaries , ed Mauche, C.W., Cambridge University Press.Google Scholar
Smak, J., 1984 Acta Astr. 34 161.Google Scholar
Tuohy, I.R., Remillard, R.A., Brissenden, R.J.V. and Bradt, H.V., 1990 Astrophys. J 359, 204.Google Scholar
White, N. E., 1989, Astr. Astrophys. Rev. 1.Google Scholar
Whitehurst, R., 1988, Mon. Not. R. astr. Soc. 232, 35.Google Scholar
Whitehurst, R. and King, A.R., 1991 Mon. Not. R. astr. Soc. 249, 25.Google Scholar