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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 | Abstract: | Recent 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 | Services: | Forum | Review | PDF | Favorites |
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