We report the detection of a type III burst in association with a dyna
mic X-ray coronal jet observed by Yohkoh/SXT. The type III burst obser
ved with the Nancay (France) multifrequency radioheliograph is spatial
ly and temporally coincident with the X-ray jet. The radio locations a
t different frequencies (236.6 and 164 MHz) are aligned along the leng
th of the jet. The observation of the type III burst in association wi
th the X-ray jet implies the acceleration of electrons to several tens
of keV, along with the heating responsible for the production of soft
X-rays. This association implies the existence of open field lines in
dense coronal structures identified on the Sun's disk. This is the fi
rst observation of dense coronal structures on the disk, along which t
ype III emitting nonthermal electrons propagate. We find that this str
ucture begins to form before the type III emission. At the time of the
type III burst we estimate a density of 6-10 x 10(8) cm(-3) for a tem
perature of similar to 5-6 MK at an altitude of 20,000 km.