2005A&A...440L..25K


Query : 2005A&A...440L..25K

2005A&A...440L..25K - Astronomy and Astrophysics, volume 440L25-28 (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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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* VW Hyi CV* 04 09 11.3967378648 -71 17 41.554528260   12.786 12.543 14.160   DQ 661 0
2 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
3 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0
4 X Aql X-1 LXB 19 11 16.0571313336 +00 35 05.868232692           ~ 1186 1

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