Dwarf Nova Oscillations and Quasi-Periodic Oscillations: Extension of the Two-QPO Diagram of X-Ray Binaries, and a new kind of DNO

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dc.creatorWarner, Brian
dc.creatorWoudt, Patrick A.
dc.date2003-01-10
dc.date.accessioned2026-07-07T02:07:08Z
dc.date.available2026-07-07T02:07:08Z
dc.descriptionSeventeen examples are given of Cataclysmic Variable (CV) stars possessing both Dwarf Nova Oscillations (DNOs) and Quasi-Periodic Oscillations (QPOs). These form an extension of the X-Ray Two-QPO correlation to frequencies three orders of magnitude lower. We draw attention to the existence of a second type of DNO in CVs, which is probably caused by magnetically channelled accretion onto the white dwarf.
dc.description6 pages, 2 figures, to appear in the proceedings of `Magnetic Cataclysmic Variables' (Cape Town, December 2002), eds. M. Cropper & S. Vrielmann
dc.identifierhttps://arxiv.org/abs/astro-ph/0301168
dc.identifierhttp://arxiv.org/abs/astro-ph/0301168
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5596
dc.subjectAstrophysics
dc.titleDwarf Nova Oscillations and Quasi-Periodic Oscillations: Extension of the Two-QPO Diagram of X-Ray Binaries, and a new kind of DNO
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