On a Site of X-ray Emission in AE Aquarii
classification
🌌 astro-ph
keywords
hypothesisx-rayadoptedanalysisaquariibrieflycurrentlydetected
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An analysis of recently reported results of XMM-Newton observations of AE Aqr within a hypothesis that the detected X-ray source is located inside the Roche lobe of the white dwarf is presented. I show this hypothesis to be inconsistent with the currently adopted model of mass-transfer in the system. Possible solutions of this problem are briefly discussed.
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