We present high time-resolution multicolour observations of the quiescent soft X-ray transient XTE J1118+480 obtained with ULTRACAM. Superimposed on the double-humped continuum g′ - and i′ -band light curves are rapid flare events which typically last a few minutes. The power density spectrum of the light curves can be described by a broken power-law model with a break frequency at ∼2 mHz or a power-law model plus a broad quasi-periodic oscillation at ∼2 mHz. In the context of the cellular automaton we estimate the size of the quiescent advection-dominated accretion flow (ADAF) region to be ∼10 4 Schwarzschild radii, similar to that observed in other quiescent black hole X-ray transients, suggesting the same underlying physics. The similarities between the low/hard and quiescent-state power density spectrum suggest a similar origin for the optical and X-ray variability, most likely from regions at or near the ADAF. © 2005 RAS.
Publication Source (Journal or Book title)
Monthly Notices of the Royal Astronomical Society
Shahbaz, T., Dhillon, V., Marsh, T., Casares, J., Zurita, C., Charles, P., Haswell, C., & Hynes, R. (2005). ULTRACAM observations of the black hole X-ray transient XTE J1118+480 in quiescence. Monthly Notices of the Royal Astronomical Society, 362 (3), 975-982. https://doi.org/10.1111/j.1365-2966.2005.09361.x