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A&A 376, L17-L21 (2001)
DOI: 10.1051/0004-6361:20011042
VLT optical observations of V821 Ara(=GX339-4) in an extended "off" state
T. Shahbaz1, R. Fender2 and P. A. Charles31 Instituto de Astrofísica de Canarias 38200 La Laguna, Tenerife, Spain
2 Astronomical Institute "Anton Pannekoek" , University of Amsterdam and Center for High Energy Astrophysics, Kruislaan, 403, 1098 SJ, Amsterdam, The Netherlands
e-mail: rpf@@astro.uva.nl
3 Department of Physics & Astronomy, University of Southampton, Southampton, SO17 1BJ, UK
e-mail: pac@astro.soton.ac.uk
(Received 6 April 2001 / Accepted 19 July 2001 )
Abstract
We report on low-resolution spectroscopy of GX339-4 during
its current, extended X-ray
"off" state in May 2000 (r=20.1) obtained with the VLT Focal Reducer/low dispersion
Spectrograph (FORS1). Although we do not positively detect the secondary star
in GX339-4 we place an upper limit of 30 percent on the contribution of a
"normal" K-type secondary star spectrum to the observed flux. Using this limit for
the observed magnitude of the secondary star, we find a lower limit for the
distance of GX339-4 to be 5.6 kpc.
Key words: stars: individual: GX339 -- 4 stars X-rays: stars accretion, accretion disks black hole physics
Offprint request: T. Shahbaz, tsh@ll.iac.es
SIMBAD Objects in preparation
© ESO 2001
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