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Radiation-hydrodynamic Models of the Accretion Spots in Magnetic Cataclysmic Variables

Published online by Cambridge University Press:  12 April 2016

K. Beuermann
K. Beuermann*
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, D-37083 Göttingen, Germany

Abstract

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The structure of the near-polar accretion spots on accreting magnetic white dwarfs has been studied theoretically and observationally in numerous papers over the last decade. Detailed treatments are available for the regime of low mass flux, usually termed the bombardment case, and for higher mass fluxes which create a strong shock standing above the photosphere of the white dwarf. No general treatment is so far available for the case of shocks buried deep in the photosphere. I review the theoretical foundations, present some applications of theory, and discuss in short the open questions which still need to be addressed.

Type
Part 3. B. Accretion Plasma diagnostics - Theory
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 187 - 200
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Aizu, k. 1973, Prog. Theor. Phys., 49, 1184 CrossRefGoogle Scholar
Beuermann, K., & Schwope, A. D. 1994, ASP Conf. Ser., 56, 119 Google Scholar
Beuermann, K. 1998, in TATA Golden Jubilee Conf. High Energy Astronomy and Astrophysics, p. 100, eds. Agrawal, P. C. & Visvanath, P. R. Google Scholar
Cropper, M., Wu, K., Ramsay, G., & Kocabiyik, A. 1999, MNRAS, 306, 684 Google Scholar
Bailey, J., Ferrano, L., & Wickramasinghe, D. T. 1991, MNRAS, 251, 37p CrossRefGoogle Scholar
Fischer, A., & Beuermann, K. 2001, A&A, 373, 211 Google Scholar
Frank, J., King, A. R., & Lasota, J.-P. 1988, A&A, 193, 113 Google Scholar
Gänsicke, B. T., Beuermann, K., de Martino, D. 1995, A&A, 303, 127 Google Scholar
Gänsicke, B. T., Hoard, D. W., Beuermann, K., et al. 1998, A&A, 338, 933 Google Scholar
Hameury, J.-M., & King, A. R. 1988, MNRAS, 235, 433 CrossRefGoogle Scholar
Imamura, J. N., Durison, R. H., Lamb, D. Q., Weast, G. J. 1987, ApJ, 313, 298 CrossRefGoogle Scholar
Lamb, D. Q., & Masters, A. R., ApJ, 234, L117 Google Scholar
Langer, S. H., Chanmugam, G., & Shaviv, G. 1982, ApJ, 258, 289 Google Scholar
Larsson, S. 1992, A&A, 265, 133 Google Scholar
Lesch, H. 1990, A&A, 239, 437 Google Scholar
King, A. R., & Lasota, J.-P. MNRAS, 188, 653 Google Scholar
Kuijpers, J., & Pringle, J. E. 1982, A&A 114, L4 Google Scholar
Priedhorsky, W., Matthews, K., Neugebauer, G., Werner, M., Krzeminski, W. 1978, ApJ, 226, 397 CrossRefGoogle Scholar
Ramsay, G., 1994, MNRAS, 270, 692 CrossRefGoogle Scholar
Rothschild, R. E., Gruber, D. E., Knight, F. K., et al. 1981, ApJ, 250, 723 Google Scholar
Saxton, C. J., Wu, K. 2001, 324, 659 Google Scholar
Stone, R. G., Tsurutani, B. T., eds. 1985, Collisionless Shocks in the Heliosphere: A Tutoral Review, Geophysical Monograph 34, American Geophysical Union, Washington D.C. Google Scholar
Tennant, A. F., Wu, K., O’Dell, S. L., Weisskopf, M. C. 1998, PASA, 15, 339 CrossRefGoogle Scholar
Woelk, U., & Beuermann, k. 1992, A&A, 256, 498 Google Scholar
Woelk, U., & Beuermann, k. 1993, A&A, 280, 169 Google Scholar
Woelk, U., & Beuermann, k. 1996, A&A, 306, 232 Google Scholar
Wu, K. 2000, Space Sci.Rev., 93, 611 Google Scholar
Wu, K., Chanmugam, G., & Shaviv, G. 1994 ApJ, 426, 664 Google Scholar
Wu, K., Cropper, M., & Ramsay, G. 2001 MNRAS, 327, 208 Google Scholar
Zheleznyakov, V. V. 1983, Ap&SS, 97, 229 Google Scholar