University of Hertfordshire

From the same journal

From the same journal

By the same authors

The curious activity in the nucleus of NGC 4151: jet interaction causing variability?

Research output: Contribution to journalArticlepeer-review

Documents

  • 2004.10552v1

    Accepted author manuscript, 393 KB, PDF document

  • D. R. A. Williams
  • R. D. Baldi
  • I. M. McHardy
  • R. J. Beswick
  • F. Panessa
  • D. May
  • J. Moldón
  • M. K. Argo
  • G. Bruni
  • B. T. Dullo
  • J. H. Knapen
  • E. Brinks
  • D. M. Fenech
  • C. G. Mundell
  • T. W. B. Muxlow
  • M. Pahari
  • J. Westcott
View graph of relations
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
DOIs
Publication statusPublished - 4 May 2020

Abstract

A key characteristic of many active galactic nuclei (AGN) is their variability, but its origin is poorly understood, especially in the radio domain. Williams et al. (2017) reported a ~50 per cent increase in peak flux density of the AGN in the Seyfert galaxy NGC 4151 at 1.5 GHz with the e-MERLIN array. We present new high resolution e-MERLIN observations at 5 GHz and compare these to archival MERLIN observations to investigate the reported variability. Our new observations allow us to probe the nuclear region at a factor three times higher-resolution than the previous e-MERLIN study. We separate the core component, C4, into three separate components: C4W, C4E and X. The AGN is thought to reside in component C4W, but this component has remained constant between epochs within uncertainties. However, we find that the Eastern-most component, C4E, has increased in peak flux density from 19.35$\pm$1.10 to 37.09$\pm$1.86 mJy/beam, representing a 8.2 sigma increase on the MERLIN observations. We attribute this peak flux density increase to continued interaction between the jet and the emission line region (ELR), observed for the first time in a low-luminosity AGN such as NGC 4151. We identify discrete resolved components at 5 GHz along the jet axis, which we interpret as areas of jet-ELR interaction.

Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Projects

ID: 21087355