  Among hard X-ray Galactic sources detected in the Swift and INTEGRAL surveys,
those discovered as accreting white dwarf binaries have suprisingly boosted in
number in the recent years. The majority are identified as magnetic Cataclysmic
Variables of the Intermediate Polar type, suggesting this subclass as an
important constituent of the Galactic population of X-ray sources. We here
review and discuss the X-ray emission properties of newly discovered sources in
the framework of an identification programme with the XMM-Newton satellite that
increased the sample of this subclass by a factor of two.
