SIMBAD references

2005A&A...440L..25K - Astronomy and Astrophysics, volume 440, L25-28 (2005/9-3)

QPOs in cataclysmic variables and in X-ray binaries.

KLUZNIAK W., LASOTA J.-P., ABRAMOWICZ M.A. and WARNER B.

Abstract (from CDS):

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.

Abstract Copyright:

Journal keyword(s): accretion, accretion discs - novae, cataclysmic variables - X-ray: binaries

Simbad objects: 4

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