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The X-ray eclipse of the dwarf nova HT Cassiopeiae observed by the<i>XMM</i>-Newton satellite: spectral and timing analysis
A cataclysmic variable is a binary system consisting of a white dwarf that accretes material from a secondary object via the Roche-lobe mechanism. In the case of long enough observation, a detailed temporal analysis can be performed, allowing the physical properties of the binary system to be determined. We present …