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Paper: X-ray emission from the post-shock flow
Volume: 157, Annapolis Workshop on Magnetic Cataclysmic Variables
Page: 309
Authors: van Teeseling, A.; Fischer, A.; Beuermann, K.
Abstract: In view of the coming AXAF, XMM and ASTRO-E high-resolution X-ray spectra, we discuss the validity of the coronal approximation for the X-ray emission from the post-shock flow in magnetic cataclysmic variables. Based on the hydrodynamical post-shock solution of Woelk & Beuermann (1996), we present angle-dependent cyclotron and X-ray spectra of a two-dimensional accretion column.
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