  Recent results are presented and discussed regarding the EUV and X-ray
emission of nonmagnetic cataclysmic variables. Emphasis is given to high
accretion rate systems (novalike variables and dwarf novae in outburst), and to
a number of apparent discrepancies between observations and the theory of the
boundary layer between the accretion disk and the surface of the white dwarf.
Discussed are EUV and X-ray light curves, dwarf nova oscillations, and spectra,
with new and previously unpublished results on SS Cyg and OY Car.
