Abstract:Results of a study of the fast timing variability of the magnetic cataclysmic variable (mCV) EX Hya are presented. It was shown that one may expect the rapid flux variability of mCVs to be smeared out at timescales shorter than the cooling time of hot plasma in the post shock region of the accretion curtain near the WD surface. Estimates of the cooling time and the mass accretion rate, thus provide us with a tool to measure the density of the post-shock plasma and the crosssectional area of the accretion funne… Show more
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