Abstract
Comparison of the period distributions of various classes of CVs confirms an extreme bias of the synchronous AM Her systems toward short orbital periods, while the DQ Her systems do not differ significantly from the distribution of non-magnetic systems. This suggests either strong selection effects or enhanced evolution of the AM Her systems. There is as yet no obvious bimodality in either the magnetic field distributions of isolated white dwards or of CV primaries. However, clear differences between the two exist: the strongest being that magnetic primaries are overrepresented among short period CVs by more than an order of magnitude in comparison to the field white dwarfs.
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Angel, J. R. P., Borra, E. F. and Landstreet, J. D. 1981,Ap. J. Suppl.,45, 457.
Chanmugam, G. and Ray, A. 1984,Ap. J.,285, 252.
King, A. R. 1985,M.N.R.A.S.,217, 23p.
King, A. R., Frank, J. and Ritter, H. 1985,M.N.R.A.S.,213, 181.
Lamb, D. Q. and Patterson, J. 1983, inCataclysmic Variables and Related Objects, eds. M. Livio and G. Shaviv, Dordrecht: Reidl.
McCook, G. P. and Sion, E. M. 1984, Villanova University Obs. Contr. No. 3, Willanova Press, Villanova PA.
Morris, S. L., Schmidt, G. D., Liebert, J., Stocke, J., Gioia, I. and Maccacaro, T. 1987,Ap. J. in press.
Ritter, H. and Burkert, A. 1986,Astr. Ap.,158, 161.
Schmidt, G. D. 1986, talk presented at the Sixth European Workshop on White Dwarfs, Rome Observatory at Monte Porzio, June 11–13, 1986, to be published in Memorie della Societa Astronomica Italiana.
Schmidt, G. D., Stockman, H. S. and Grandi, S. 1986.Ap. J.,300, 804.
Shafter, A. W. Szkody, P. and Thorstenson, J.Ap. J., in press.
Shafter, A. W., Szkody, P., Liebert, J., Penning, W. R., Bond, H. E., and Grauer, A. D. 1986,Ap. J.,290, 707.
Verbunt, F. and Zwaan, C. 1981,Astr. Ap.,100 L7.
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Schmidt, G.D., Liebert, J. The period and magnetic field distributions of cataclysmic variables: Implications for their evolution. Astrophys Space Sci 131, 549–555 (1987). https://doi.org/10.1007/BF00668137
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DOI: https://doi.org/10.1007/BF00668137