Magnetic Cataclysmic Variables discovered in hard X-rays

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dc.contributor.authorFalanga, M.
dc.contributor.authorde Martino, D.
dc.contributor.authorBernardini, F.
dc.contributor.authorMukai, K.
dc.date.accessioned2019-11-14T17:42:30Z
dc.date.available2019-11-14T17:42:30Z
dc.date.issued2019-06-27
dc.descriptionProceedings of the 12th INTEGRAL conference and 1st AHEAD Gamma-ray Workshop, Geneva (Switzerland), 11-15 February 2019,
dc.description.abstractAmong hard X-ray galactic sources detected by INTEGRAL and Swift surveys, those discovered as accreting white dwarfs have surprisingly boosted in number, representing 20% of the galactic sample. The majority are identified as magnetic cataclysmic variabiles of the intermediate polar type suggesting this subclass as an important constituent of galactic population of X-ray sources. In this conference-proceeding, we review the X-ray emission properties as observed with our ongoing XMM-Newton programme of newly discovered INTEGRAL and/or Swift sources that enlarged almost by a factor of two, identifying cataclysmic variabiles commonalities and outliers.en_US
dc.description.sponsorshipDdM acknowledges financial suport from INAF-ASI agreements I/037/12/0 and ASI-INAF n.2017-14-H.0 and INAF-PRIN SKA/CTA Presidential Decree 70/2016. FB is founded by the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement n. 664931.en_US
dc.description.urihttps://arxiv.org/abs/1906.11612en_US
dc.format.extent6 pagesen_US
dc.genreconference papers and proceedings preprintsen_US
dc.identifierdoi:10.13016/m2zrqo-kxfw
dc.identifier.citationFalanga, M.; de Martino, D.; Bernardini, F.; Mukai, K.; Magnetic Cataclysmic Variables discovered in hard X-rays (2019); https://arxiv.org/abs/1906.11612en_US
dc.identifier.urihttp://hdl.handle.net/11603/16306
dc.language.isoen_USen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.subjectnovaeen_US
dc.subjectcataclysmic variablesen_US
dc.subjectwhite dwarfsen_US
dc.subjectX-raysen_US
dc.subjectbinariesen_US
dc.subjectpopulationsen_US
dc.titleMagnetic Cataclysmic Variables discovered in hard X-raysen_US
dc.typeTexten_US

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