GX 339-4 in a very low luminosity state
ATel #196; Elena Gallo, Rob Fender (U Amsterdam) & Stephane Corbel (U Paris VII & CEA Saclay)
on 3 Oct 2003; 15:48 UT
Credential Certification: Elena Gallo (egallo@science.uva.nl)
Subjects: Radio, X-ray, Black Hole, Transient
A 30 ksec Chandra ACIS-S observation on MJD 52911 reveals the black hole X-ray
binary GX 339-4 to have entered a very low luminosity state following a more
than 2-year-long outburst period (ATEL #85, #95, #107, #120).
The X-ray spectrum is well fitted by an absorbed power-law with photon index
2+/-0.2 and absorption column N_H=7+/-1x10e21 cm^-2. The (unabsorbed)
0.4-11 keV flux is of 3.8e-13 erg sec^-1 cm^-2, with a corresponding
luminosity of 4.6e31x(d/kpc)^2 erg sec^-1, comparable to the faintest ever
measured from GX 339-4.
Simultaneous radio observations with the Australia Telescope Compact Array
did not detect the source to an rms noise level of 0.015 mJy/beam at 4.8 GHz.