Williams, D. R. A.D. R. A.WilliamsMcHardy, I. M.I. M.McHardyBALDI, RANIERI DIEGORANIERI DIEGOBALDIBeswick, R. J.R. J.BeswickPahari, M.M.PahariArgo, M. K.M. K.ArgoBeri, A.A.BeriBoorman, P.P.BoormanBrinks, E.E.BrinksDullo, B. T.B. T.DulloFenech, D. M.D. M.FenechIneson, J.J.InesonKharb, P.P.KharbKnapen, J. H.J. H.KnapenMuxlow, T. W. B.T. W. B.MuxlowWestcott, J.J.Westcott2022-07-142022-07-1420190035-8711http://hdl.handle.net/20.500.12386/32481We 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 ∼4 arcsec (∼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 ∼3 arcmin (∼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 be chance associations due to high source 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.STAMPAenArticle10.1093/mnras/stz1135https://academic.oup.com/mnras/article/486/4/4962/54820842019MNRAS.486.4962WFIS/05 - ASTRONOMIA E ASTROFISICA