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 oscillation harmonics that are seen in some neutron star and black holes X-Ray binaries. We point out that the behaviour of the dwarf nova WZ Sge has some similarities to those of accreting millisecond pulsars.
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机译：我们比较灾难性变量和X射线二进制文件中快速振荡的一些特性。除了早期的识别外，两种类型在高低频率准周期性振荡之间具有相同的相关性，我们现在发现矮人Nova VW Hyi在其后期突出的突出阶段显示为1：2：3振荡谐波在一些中子星和黑洞X射线二进制文件中看到。我们指出，Dwarf Nova WZ SGE的行为与毫秒脉冲脉冲的相似性。
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