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

Williams, D; McHardy, I; Baldi, R; Beswick, R; Pahari, M; Argo, M; Beri, A; Boorman, P; Brinks, E; Dullo, B; Fenech, D; Ineson, J; Kharb, P; Knapen, J; Muxlow, T; Westcott, J

Journal article

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

Abstract:: 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 ∼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.

Publication status:: Published

Peer review status:: Peer reviewed

Actions

Email

Email this record

Send the bibliographic details of this record to your email address.

Your Email
Please enter the email address that the record information will be sent to.

-
Your message (optional)
Please add any additional information to be included within the email.
Cite

Cite this record

APA Style

Williams, D., McHardy, I., Baldi, R., Beswick, R., Pahari, M., Argo, M., Beri, A., Boorman, P., Brinks, E., Dullo, B., Fenech, D., Ineson, J., Kharb, P., Knapen, J., Muxlow, T., & Westcott, J. (2019). Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA. Monthly Notices of the Royal Astronomical Society, 486(4), 4962–4979.

MLA Style

Williams, D., et al. “Unveiling the 100 Pc Scale Nuclear Radio Structure of NGC 6217 with e-MERLIN and the VLA.” Monthly Notices of the Royal Astronomical Society, vol. 486, no. 4, Oxford University Press, 2019, pp. 4962–79.

Chicago Style

Williams, D, I McHardy, R Baldi, R Beswick, M Pahari, M Argo, A Beri, et al. 2019. “Unveiling the 100 Pc Scale Nuclear Radio Structure of NGC 6217 with e-MERLIN and the VLA.” Monthly Notices of the Royal Astronomical Society 486 (4): 4962–79.
Share
Print