Accretion Column Structure of Magnetic Cataclysmic Variables from X-Ray Spectroscopy

Using Chandra HETG data, we present light curves for individual spectral lines of Mg XI and Mg XII for EX Hydrae, an intermediate polar-type cataclysmic variable. The Mg XI light curve, folded on the white dwarf spin period, shows two spikes that are not seen in the Mg XII or broadband light curves. Occultation of the accretion column by the body of the white dwarf would produce such spikes for an angle between the rotation axis and the accretion columns of α = 18° and a height of the Mg XI emission above the white dwarf surface of ≲0.0004 white dwarf radii, or ≲4 km. The absence of spikes in the Mg XII and broadband light curves could then be explained if the bulk of its emission forms at much larger height, more than 0.004 white dwarf radii or over 40 km, above the white dwarf surface, although this is not consistent with the predictions of the standard Aizu model of the accretion column.