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Simulation of Doppler H-alpha tomogram of the nova-like star AE Aquariisuggests that the dipole magnetic moment of the white dwarf is close to 1.5E+34G cm^3. This is consistent with the lower limit to the magnetic field strengthof the white dwarf derived from observations of circularly polarized opticalemission of the system. The rapid braking of the white dwarf and the nature ofpulsing hard X-ray emission recently detected with SUZAKU space telescope underthese conditions can be explained in terms of spin-powered pulsar mechanism. Aquestion about the origin of strongly magnetized white dwarf in the systemremains, however, open. Possible evolutionary tracks of AE Aquarii are brieflydiscussed.

AE Aquarii: The first white dwarf in the family of spin-powered pulsars