The duty cycle of radio galaxies revealed by LOFAR: Remnant and restarted radio source populations in the Lockman Hole

Stanislav S. Shabala*, Nika Jurlin, Raffaella Morganti, Marisa Brienza, Martin J. Hardcastle, Leith E. H. Godfrey, Martin G. H. Krause, Ross J. Turner

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

51 Citations (Scopus)
121 Downloads (Pure)

Abstract

Feedback from radio jets associated with active galactic nuclei (AGNs) plays a profound role in the evolution of galaxies. Kinetic power of these radio jets appears to show temporal variation, but the mechanism(s) responsible for this process are not yet clear. Recently, the LOw Frequency ARray (LOFAR) has uncovered large populations of active, remnant, and restarted radio jet populations. By focusing on LOFAR data in the Lockman Hole, in this work we use the Radio AGNs in Semi-Analytic Environments (RAiSE) dynamical model to present the first self-consistent modelling analysis of active, remnant, and restarted radio source populations. Consistent with other recent work, our models predict that remnant radio lobes fade quickly. Any high (> 10 per cent) observed fraction of remnant and restarted sources therefore requires a dominant population of short-lived jets. We speculate that this could plausibly be provided by feedback-regulated accretion.

Original languageEnglish
Pages (from-to)1706-1717
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume496
Issue number2
DOIs
Publication statusPublished - Aug-2020

Keywords

  • galaxies: active
  • galaxies: jets
  • radio continuum: galaxies
  • ACTIVE GALACTIC NUCLEI
  • SUPERMASSIVE BLACK-HOLES
  • STAR-FORMATION
  • RELATIVISTIC JETS
  • PARTICLE CONTENT
  • HOST GALAXIES
  • AGN ACTIVITY
  • LOUD AGN
  • FEEDBACK
  • GAS

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