  The black hole candidate GX 339-4 was first detected as a variable radio
source by Sood & Campbell-Wilson in May 1994 with the Molonglo Observatory
Synthesis Telescope (MOST). Since then, several observations have been obtained
with the Australian Telescope Compact Array (ATCA) in order to study the radio
behavior of this source in relation to its soft and hard X-ray activity. We
present new results of high resolution radio observations performed with the
ATCA in order to study the jet-like feature observed in GX 339-4 by Fender et
al (1997). From the ATCA lightcurve at 8640 MHz, we find evidence of quenched
radio emission from GX 339-4.
