Falanga, M.de Martino, D.Bernardini, F.Mukai, K.2019-11-142019-11-142019-06-27Falanga, M.; de Martino, D.; Bernardini, F.; Mukai, K.; Magnetic Cataclysmic Variables discovered in hard X-rays (2019); https://arxiv.org/abs/1906.11612http://hdl.handle.net/11603/16306Proceedings of the 12th INTEGRAL conference and 1st AHEAD Gamma-ray Workshop, Geneva (Switzerland), 11-15 February 2019,Among 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.6 pagesen-USThis 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.novaecataclysmic variableswhite dwarfsX-raysbinariespopulationsText