The Emission from Post-Shock Flows in mCVs
classification
🌌 astro-ph
keywords
emissionmcvspost-shockstructureverticalx-rayaccountaccretion
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We re-examine the vertical structure of the post-shock flow in the accretion region of mCVs, and the X-ray emission as a function of height. We then predict X-ray light curves and phase-resolved spectra, taking into account the vertical structure, examine the implications and check whether the predicted heights are compatible with observation.
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