The quiescent optical light curve of XTE J2123-058
T. Shahbaz(IAC, Spain) C. Zurita (IAC, Spain), J. Casares (IAC, Spain), G. Dubus (Caltech, USA) P.A. Charles (Southampton, UK) R. Mark Wagner (Arizona, USA) E. Ryan (Arizona, USA)
Abstract
We present optical photometry of the X-ray transient XTE J2123-058
during its quiescent state taken in 1999 and 2000.
We fit the R-band light curves with a model which requires the ellipsoidal
modulation and X-ray heating of the Roche-lobe filling secondary star,
and an accretion disc bulge, i.e. where the gas stream impacts the
accretion disc. The observed lack of light near phase 0.8 is interpreted
as the eclipse of inner parts of the accretion disc by the bulge.
This scenario is highly plausible given the high binary inclination
of the system.
Our fits allow us to constrain the size of the accretion
disc to lie in the range 0.26-0.56
(68 percent confidence).
Using the distance of 9.3 kpc and the X-ray flux inferred from the
heated hemisphere of the companion, we
obtain an unabsorbed X-ray luminosity of 1.2
ergs-1
for XTE J2123-058 in quiescence. From the observed quiescent optical/IR
colours we find that the power-law index (-1.4) for the spectral
distribution of the accretion disc compares well with other quiescent
X-ray transients.
CATEGORY: BLACK HOLE AND NEUTRON STAR BINARIES