J. Homan et al., A variable 0.58-2.44 Hz quasi-periodic oscillation in the eclipsing and dipping low-mass X-ray binary EXO 0748-676, ASTROPHYS J, 516(2), 1999, pp. L91-L94
We report the discovery of a quasi-periodic oscillation (QPO) in data obtai
ned with the Rossi X-Ray Timing Explorer of the dipping and eclipsing low-m
ass X-ray binary EXO 0748-676. The QPO had a frequency between 0.58 and 2.4
4 Hz changing on timescales of a few days and an rms amplitude between 8% a
nd 12%, and it was detected in the persistent emission during dips and duri
ng type I X-ray bursts. During one observation, when the count rate was a f
actor of 2-3 higher than otherwise, the QPO was not detected. The strength
of the QPO did not significantly depend on photon energy and is consistent
with being the same in the persistent emission, both during and outside the
dips and during type I X-ray bursts. Frequency shifts were observed during
three of the four X-ray bursts. We argue that the QPO is produced by the s
ame mechanism as the QPO recently found by Jonker et al. in 4U 1323-62. Alt
hough the exact mechanism is not clear, it is most likely related to the hi
gh inclination of both systems. An orbiting structure in the accretion disk
that modulates the radiation from the central sourer seems the most promis
ing mechanism.