Bibcode
Shahbaz, T.; Fender, R.; Charles, P. A.
Referencia bibliográfica
Astronomy and Astrophysics, v.376, p.L17-L21 (2001)
Fecha de publicación:
9
2001
Revista
Número de citas
51
Número de citas referidas
45
Descripción
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. Based on observations performed at the
European Southern Observatory, Paranal, Chile.