Evolution of Cataclysmic Binaries

  • Bohdan Paczyński
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUH, volume 8)

Abstract

The minimum period of hydrogen rich cataclysmic binaries at about 80 minutes is due to evolution driven by gravitational radiation. The nature of the cap between 2 and 3 hour periods is less clear. Magnetic braking may be responsible, but this would be in contradiction with the hibernating nova scenario. It is interesting that contact binaries of W UMa type are subject to little or no magnetic braking.

Keywords

Mass Transfer Rate White Dwarf Gravitational Radiation Cataclysmic Variable High Mass Transfer 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Bragaglia, A., Greggio, L., Renzini, A., and D’Odorico, S. 1988, The Messenger, No. 52, p. 35.ADSGoogle Scholar
  2. Eggleton, P. P. 1976, IAU Symp. 73, p. 209, Eds: P. P. Eggleton, S. Mitton, and J. A. J. Whelan, (D. Reidel Publ. Co.).Google Scholar
  3. Fruchter, A. S., Stinebring, D. R., and Taylor, J. H. 1988, Nature, 333, 237.ADSCrossRefGoogle Scholar
  4. Fujimoto, M. Y. 1982, Ap. J., 257, 767.ADSCrossRefGoogle Scholar
  5. Griffin, R. F. 1988, The Observatory, 108, 90.ADSGoogle Scholar
  6. Hameury, J. M., King, A. R., Lasota, J. P., and Ritter, H. 1987, Ap. J., 316, 275.ADSCrossRefGoogle Scholar
  7. Hameury, J. M., King, A. R., Lasota, J. P., and Ritter, H. 1988a, Mon. Not. R. astr. Soc. 231, 535.ADSGoogle Scholar
  8. Hameury, J. M., King, A. R., and Lasota, J. P. 1988b, Astron. Ap., 195, L12.ADSGoogle Scholar
  9. Iben, I. Jr., and Tutukov, A. V. 1984, Ap. J. Suppl., 54, 535.ADSCrossRefGoogle Scholar
  10. Kafuzny, J. 1988, private communication.Google Scholar
  11. Kafuzny, J., and Shara, M. M. 1987, Ap. J., 314, 585.ADSCrossRefGoogle Scholar
  12. King, A. R. 1988, Quarterly J. R. A. S., 29, 1.ADSGoogle Scholar
  13. Kutter, G. S., and Sparks, W. M. 1980, Ap. J., 239, 988.ADSCrossRefGoogle Scholar
  14. Lamb, D. Q., and Patterson, J. 1983, IAU Coll. No 72, p. 229, Eds: M. Livio and G. Shaviv, (D. Reidel Publ. Co.).Google Scholar
  15. Liebert, J., and Stockman, H. S. 1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, p. 151, Eds: D. Q. Lamb and J. Patterson, (D. Reidel Publ. Co.).Google Scholar
  16. MacDonald, J. 1986, Ap. J., 305, 251.Google Scholar
  17. Mayor, M. 1980, Astron. Ap., 87, Ll.Google Scholar
  18. Molnar, L. A. 1988, Ap. J. (Letters), 331, L25.ADSCrossRefGoogle Scholar
  19. Motch, C., Pedersen, H., Beuermann, K., Pakull, M. W., and Courvoisier, T. J.-L. 1988, Ap. J., 313, 792.Google Scholar
  20. Paczynski, B. 1981, Acta Astron., 31 1.Google Scholar
  21. Paczynski, B., and Sienkiewicz, R. 1981, Ap. J. (Letters), 248, L27.Google Scholar
  22. Paczynski, B., and Sienkiewicz, R. 1983, Ap. J., 268, 825.Google Scholar
  23. Paczynski, B. 1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, p. 1, Eds: D. Q. Lamb and J. Patterson, (D. Reidel Publ. Co.).Google Scholar
  24. Patterson, J. 1984, Ap. J. Suppl, 54, 443.Google Scholar
  25. Phinney, E. S., Evans, C. R., Blandford, R. D., and Kulkarni, S. R. 1988, Nature, 333, 832.ADSCrossRefGoogle Scholar
  26. Prialnik, D., Livio, M., Shaviv, G., and Kovetz, A. 1982, Ap. J., 257 , 312.Google Scholar
  27. Prialnik, D., and Shara, M. M. 1986, Ap. J., 311, 172.ADSCrossRefGoogle Scholar
  28. Rappaport, S., Joss, P. C., and Webbink, R. F. 1982, Ap. J., 254, 616.ADSCrossRefGoogle Scholar
  29. Ritter, H. 1987, Astron. Ap. Suppl., 70. 335.ADSGoogle Scholar
  30. Robinson, E. L., and Shafter, A. W. 1987, Ap. J., 322, 296.ADSCrossRefGoogle Scholar
  31. Rucinski, S. M. 1985, in Interacting binary stars, p. 113, Eds: J. E. Pringle and R. A. Wade, (Cambridge University Press).Google Scholar
  32. Saffer, R. A., Liebert, J., and Olszewski, W. 1988, Ap. J., 334, ...Google Scholar
  33. Schmidtke, P. C., and Cowley, A. P. 1987, Astron. J., 93, 374.ADSCrossRefGoogle Scholar
  34. Shara, M. M. 1988, 20th General Assembly, IAU, Joint Discussion II, this volume.Google Scholar
  35. Shara, M. M., Livio, M., Moffat, A. F. J., and Orio, M. 1986, Ap. J., 311, 163.ADSCrossRefGoogle Scholar
  36. Spruit, H. C., and Ritter, H. 1983, Astron. Ap., 124, 267.ADSGoogle Scholar
  37. Tutukov, A. V., and Yungelson, L. R. 1979, Acta Astron., 29, 665.ADSGoogle Scholar
  38. Verbunt, F. 1984, Mon. Not. R. astr. Soc., 209, 227.ADSGoogle Scholar
  39. Verbunt, F., and Zwaan, C. 1981, Astron. Ap., 100, L7.ADSGoogle Scholar
  40. Webbink, R. E. 1979, in White Dwarfs and Variable Degenerate Stars, Ed.: H. M. Van Horn and V. Weidemann ( New York: University of Rochester Press ), p. 426.Google Scholar
  41. Wolff, S. C. 1978, Ap. J., 222, 559.ADSCrossRefGoogle Scholar

Copyright information

© International Astronomical Union 1989

Authors and Affiliations

  • Bohdan Paczyński
    • 1
  1. 1.Department of AstrophysicsPrinceton UniversityPrincetonUSA

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