No CrossRef data available.
Article contents
Magnetic Braking and Its Implication for CV Evolution
Published online by Cambridge University Press: 25 April 2016
Abstract
We review the models of magnetic braking for synchronously rotating magnetic cataclysmic variables, and discuss the implications of magnetic braking for orbital evolution and the upper limit to the magnetic fields (about 70 MG) of the observed AM Herculis systems.
Keywords
- Type
- Magnetic Fields, Disks and Jets: A Workshop organised by the ANU Astrophysical Theory Centre The ANU Astrophysical Theory Centre
- Information
- Publications of the Astronomical Society of Australia , Volume 13 , Issue 1 , January 1996 , pp. 81 - 86
- Copyright
- Copyright © Astronomical Society of Australia 1996
References
Beuerman, K.
1995, in Proceedings of the Cape Town Workshop on Magnetic Cataclysmic Variables, in pressGoogle Scholar
Liebert, J., & Stockman, H. S.
1985, in Cataclysmic Variables and Low-Mass X-Ray Binaries, ed. Lamb, D. Q. & Patterson, J. (Dordrecht: Reidel), 151
Google Scholar
Mestel, L.
1984, in Cool Stars, Stellar Systems and the Sun, ed. Baliunas, S. L. & Hartmann, L. (Heidelberg:Springer-Verlag), 49
Google Scholar
Schmidt, G. D., West, S. C, Liebert, J., Green, R. F., & Stockman, H. S.
1986, ApJ, 309, 218
Google Scholar
Wickramasinghe, D. T.
1988, in Polarized Radiation of Circumstellar Origin, ed. Coyne, G. V.
Magalhaes, A. M.
Moffat, A. F. J.
Schulte-Ladback, R. E., Tapia, S. & Wickramasinghe, D. T. (Vatican City: Vatican Observatory Press), 3
Google Scholar