  A new magnetic, eclipsing cataclysmic variable is identified as the
counterpart of the X-ray source RX J0719.2+6557 detected during the ROSAT
all-sky survey. The relative phasing of photometric and spectroscopic periods
indicates a self-eclipsing system. Doppler tomography points to the heated
surface of the secondary as a strong source of emission and of diskless
accretion. Near-infrared spectroscopy revealed two unusual strong emission
features originating on the heated side of the secondary.
