Abstract
We argue that the polarised optical emission from AM Herculis-type systems arises from a compact high temperature (T≳10 keV) region closely associated with the accretion shock.
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Barrett, P. E., and Chanmugam, G.: 1984,Astrophys. J. 278, 298.
Latham, D. W., Liebert, J. and Steiner, J. E.: 1981,Astrophys. J. 246, 919.
Meggitt S. M. A. and Wickramasinghe, D. T., 1982,Monthly Notices Roy. Astron. Soc. 198, 71.
Stockman, H. S., Foltz, C. B., Schmidt, G. D., and Tapia, S.: 1983,Astrophys. J.,271, 725.
Wickramasinghe, D. T. and Meggitt, S. M. A.: 1982,Monthly Notices Roy. Astron. Soc. 198 975.
Wickramasinghe, D. T. and Visvanathan, N. V.: 1980,Monthly Notices Roy. Astron. Soc. 191 589.
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Wickramasinghe, D.T., Meggitt, S. The electron temperature of AM Herculis type systems. Astrophys Space Sci 118, 287–289 (1986). https://doi.org/10.1007/BF00651137
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DOI: https://doi.org/10.1007/BF00651137