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19 April 2024
 
  » arxiv » astro-ph/0503151

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QPOs in Cataclysmic Variables and in X-ray Binaries
Wlodek Kluzniak ; Jean-Pierre Lasota ; Marek A. Abramowicz ; Brian Warner ;
Date 7 Mar 2005
Subject astro-ph
AbstractRecent observations, reported by Warner and Woudt, of Dwarf Nova Oscillations (DNOs) exhibiting frequency drift, period doubling, and 1:2:3 harmonic structure, can be understood as disc oscillations that are excited by perturbations at the spin frequency of the white dwarf or of its equatorial layers. Similar quasi-periodic disc oscillations in black hole low-mass X-ray binary (LMXB) transients in a 2:3 frequency ratio show no evidence of frequency drift and correspond to two separate modes of disc oscillation excited by an internal resonance. Just as no effects of general relativity play a role in white dwarf DNOs, no stellar surface or magnetic field effects need be invoked to explain the black hole QPOs.
Source arXiv, astro-ph/0503151
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