Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA

We present. high-sensitivity 1,51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) radio images of the nearby galaxy NGC 6217. We resolve the compact radio source at the centre of NGC 6217 for the first time, finding a twin-lobed structure with a total linear size of similar to 4 arcsec (similar to 400 pc). The radio source does not have a compact central core, but there is an unresolved hotspot near the outer edge of the southern lobe. Combining our e-MERLIN data with new VLA (Very Large Array) A-Array data and archival multiwavelength data, we explore possible scenarios which might explain this complex radio morphology. We conclude that this radio source is most likely powered by a low-luminosity active galactic nucleus but with a possible important contribution from nuclear star formation. We also investigate the origin of a putative X-ray jet in NGC 6217, previously suggested in the literature. This 'jet- consists of three X-ray 'knots' in a line, pointed away from the nucleus, with a total size of similar to 3 arcmin (similar to 15 kpc). We find no extended radio emission coincident with the 'jet-. An additional compact radio source, aligned with the knots but without an X-ray counterpart is detected. We detect infrared/optical sources falling within the X-ray extraction regions of the 'knots', but note that these sources could he chance associations due to high soiu-ce density around the target field and we estimate the probability of three randomly aligned X-ray sources to be 0.3 per cent in this field.