SUBARU and e-Merlin observations of NGC3718. Diaries of an SMBH recoil?

Abstract

NGC3718 is a LINER $L1.9$ galaxy, lying at a distance of about $\sim 17.4$ Mpc away from earth and its similarities with NGC5128 often award it the name "northern Centaurus A". We use high angular resolution ($\sim 100$ mas) e-Merlin radio and SUBARU NIR ($\sim 170$ mas) data, to take a detailed view of the processes taking place in its central region. In order to preserve some objectivity in our interpretation, we combine our results with literature values and findings from previous studies. Our NIR maps suggest, on one hand, that towards the stellar bulge there are no large scale absorption phenomena caused by the apparent dust lane and, on the other, that there is a significant (local) contribution from hot ($\sim 1000$ K) dust to the nuclear NIR emission. The position where this takes place appears to be closer to the offset compact radio emission from our e-Merlin $6$ cm map, lying offset by $\sim 4.25$ pc from the center of the underlying stellar bulge. The shape of the radio map suggests the presence of one (or possibly two, forming an X-shape) bipolar structure(s) $\sim 1$ ($\sim 0.6$) arcsec across, which combined with the balance between the gas and the stellar velocity dispersions and the presence of hard X-ray emission, point towards effects expected by AGN feedback. We also argue that NGC3718 has a "core" in its surface brightness profile, despite the fact that it is a gas-rich galaxy and we discuss its mixed photometric and spectroscopic characteristics. The latter combined with the observed spatial and radio offsets, the relative redshift between the broad and the narrow $H\alpha$ line, the limited star formation activity and AGN feedback, strongly imply the existence of an SMBH recoil. Finally, we discuss a possible interpretation, that could naturally incorporate all these findings into one physically consistent picture.

arXiv comment18 pages, 18 figures, 3 tables, accepted for publications in A&A

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• Electromagnetic Counterparts to Massive Black Hole Mergers
• The puzzling case of the radio-loud QSO 3C 186: a gravitational wave recoiling black hole in a young radio source?
• Optical spectroscopy of local type-1 AGN LINERs
• Study of Swift/BAT Selected Low-luminosity Active Galactic Nuclei Observed with Suzaku
• The recoiling black hole candidate 3C 186: spatially-resolved quasar feedback and further evidence of a blue-shifted broad line region
• The quest for the largest depleted galaxy core: supermassive black hole binaries and stalled in-falling satellites
• Characterizing the velocity of a wandering black hole and properties of the surrounding medium using convolutional neural networks
• Constraining X-ray reflection in the low-luminosity AGN NGC 3718 using NuSTAR and XMM--Newton
• Hypercompact stellar clusters: morphological renditions and spectro-photometric models
• Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186
• Connecting the dots: Tracing the evolutionary pathway of Polar Ring Galaxies in the cases of NGC 3718, NGC 2685, and NGC 4262