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The electron temperature of AM Herculis type systems

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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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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

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