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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8420
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dc.contributor.authorSharma, Rahul-
dc.contributor.authorJain, Chetana-
dc.contributor.authorPaul, Biswajit-
dc.contributor.authorDutta, Anjan-
dc.contributor.authorRana, Vikram-
dc.date.accessioned2025-08-01T06:38:45Z-
dc.date.available2025-08-01T06:38:45Z-
dc.date.issued2025-07-10-
dc.identifier.citationThe Astrophysical Journal, 2025, Vol.987, p117en_US
dc.identifier.urihttp://hdl.handle.net/2289/8420-
dc.descriptionOpen Accessen_US
dc.description.abstractThe detection and characterization of periodic X-ray signals are crucial for identifying new compact objects and studying the mechanisms powering their emission. We report on the timing and spectral variability of CXOU J204734.8+300105, a proposed eclipsing polar-type cataclysmic variable (CV) candidate. This source has been observed once with Chandra and twice with XMM-Newton, revealing several intriguing and conflicting features in its X-ray emission. The Chandra observation showed a periodicity of ∼6000 s with an eclipse-like feature. The X-ray light curve from the 2017 XMM-Newton observation showed a period of ∼2000 s without any apparent eclipse, while the simultaneous optical light curve from the Optical Monitor showed a period of ∼6000 s. This variability raises questions about the true nature of the source. Spectral analysis indicates a multicomponent emission and emission lines due to Fe. The spectral characteristics are consistent with those observed in other CV systems. Additionally, we identified optical and near-infrared counterparts from various catalogues. Our findings suggest a dynamic and evolving accretion environment of CXOU J204734.8+300105.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2025arXiv250511322S/abstracten_US
dc.relation.urihttps://arxiv.org/abs/2505.11322en_US
dc.relation.urihttps://inspirehep.net/literature/2922095en_US
dc.relation.urihttps://doi.org/10.3847/1538-4357/addc5ben_US
dc.rights2025 The Authro(s)en_US
dc.titleIntriguing Nature of AM Her–type Candidate CXOU J204734.8+300105en_US
dc.typeArticleen_US
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