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Deep ROSAT PSPC and HRI observations of the nuclear starburst, UV flatspectrum 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 inthe same direction, giving further evidence for a one-sided X-ray jetinterpretation of this feature. It's X-ray spectrum is harder than that ofNGC6217 and the luminosity in the 0.5-2.0 keV band ~1.7 E39 erg\s. We compareour findings to parameters of other X-ray jets from other active galaxies. Wealso give positions of a total of 91 X-ray sources detected in the field to alimiting 0.5-2.0 keV flux of ~2.2E-15 erg\cm**2\s and propose optical and radioidentifications. Some of these sources have been identified in the RIXOSprogram.

A possible X-ray jet from the starburst galaxy NGC 6217