Falanga, M.M.FalangaDE MARTINO, DomitillaDomitillaDE MARTINOBernardini, F.F.BernardiniMukai, K.K.Mukai2020-12-282020-12-2820190037-8720http://hdl.handle.net/20.500.12386/29253Among 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.STAMPAenConference paperhttp://sait.oat.ts.astro.it/MSAIt9001-0219/index.html2019MmSAI..90..126FFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering