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

Authors
  • Warner, Brian
  • Woudt, Patrick A.
Type
Preprint
Publication Date
Jan 10, 2003
Submission Date
Jan 10, 2003
Identifiers
arXiv ID: astro-ph/0301168
Source
arXiv
License
Unknown
External links

Abstract

Seventeen 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.

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