  Deep ROSAT PSPC and HRI observations of the nuclear starburst, UV flat
spectrum spiral NGC6217 reveal a jet-like X-ray filament extending out 2.7'
(18.8 kpc) to the SW of the galaxy. Radio images of NGC6217 show an extent in
the same direction, giving further evidence for a one-sided X-ray jet
interpretation of this feature. It's X-ray spectrum is harder than that of
NGC6217 and the luminosity in the 0.5-2.0 keV band ~1.7 E39 erg\s. We compare
our findings to parameters of other X-ray jets from other active galaxies. We
also give positions of a total of 91 X-ray sources detected in the field to a
limiting 0.5-2.0 keV flux of ~2.2E-15 erg\cm**2\s and propose optical and radio
identifications. Some of these sources have been identified in the RIXOS
program.
