Rapid Oscillations in Cataclysmic Variables, and a Comparison with X-Ray   Binaries
  We compare some of the properties of rapid oscillations in cataclysmic variables and X-Ray binaries. In addition to the earlier recognition that both types possess the same correlation between high and low frequency quasi-periodic oscillations, we have now found that the dwarf nova VW Hyi in its late stages of outburst shows the 1:2:3 oscillations harmonics that are seen in some neutron star and black hole X-Ray binaries. We point out that the behaviour of the dwarf nova WZ Sge has some similarities to those of accreting millisecond pulsars. 
Brian Warner (Univ. of Cape Town) and Patrick A. Woudt (Univ. of Cape   Town)