Rapid Oscillations in Cataclysmic Variables, and a Comparison with X-Ray Binaries

Brian Warner; Patrick A. Woudt

doi:10.1063/1.2130244

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arXiv · astro-ph/0409026

Rapid Oscillations in Cataclysmic Variables, and a Comparison with X-Ray Binaries

Brian Warner·Patrick A. Woudt

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Abstract

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.

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Brian Warner, Patrick A. Woudt. 2004-09-01. Rapid Oscillations in Cataclysmic Variables, and a Comparison with X-Ray Binaries. https://doi.org/10.1063/1.2130244

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