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Echoes in X-ray binaries

O'Brien, K.; Horne, Keith; Hynes, R.I.; Chen, W.; Haswell, C.A. and Still, M.D. (2002). Echoes in X-ray binaries. Monthly Notices of the Royal Astronomical Society, 334(2) pp. 426–434.

DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1046/j.1365-8711.2002.05530.x
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Abstract

We present a method of analysing the correlated X-ray and optical/UV variability in X-ray binaries, using the observed time delays between the X-ray driving light curves and their reprocessed optical echoes. This allows us to determine the distribution of reprocessing sites within the binary. We model the time-delay transfer functions by simulating the distribution of reprocessing regions, using geometrical and binary parameters. We construct best-fitting time-delay transfer functions, showing the regions in the binary responsible for the reprocessing of X-rays. We have applied this model to observations of the soft X-ray transient GRO J1655-40. We find that the optical variability lags the X-ray variability with a mean time delay of 19.3±2.2 s. This means that the outer regions of the accretion disc are the dominant reprocessing site in this system. On fitting the data to a simple geometric model, we derive a best-fitting disc half-opening angle of
, which is similar to that observed after the previous outburst by Orosz & Bailyn. This disc thickening has the effect of almost entirely shielding the companion star from irradiation at this stage of the outburst.

Item Type: Journal Article
ISSN: 1365-2966
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 4416
Depositing User: Users 6827 not found.
Date Deposited: 06 Jul 2006
Last Modified: 11 Jul 2013 15:28
URI: http://oro.open.ac.uk/id/eprint/4416
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