The diverse morphologies and evolution of low-luminosity edge-brightened radio galaxies
Year: 2026
Type: article
Abstract: ABSTRACT Fanaroff–Riley class I (FRI) radio galaxies show centre-brightened emission from disrupted lower power jets, while traditionally more luminous class II (FRIIs), are edge-brightened, with relativistic jets terminating in hotspots. Population studies of radio-loud AGN (RLAGN) with low frequency, deep, wide-field surveys have revealed FRII-like radio structures at lower luminosities. We present the first high-resolution morphological investigation of a representative LOw Frequency ARray (LOFAR)-selected sample of low-luminosity FRIIs, to determine whether this new population is physically distinct from traditional high-luminosity FRIIs. Using new 1.5-GHz Jansky Very Large Array observations for a sample of 19 low-luminosity FRIIs, from the LOFAR Two Metre Sky Survey Data Release 1, with luminosities up to three orders of magnitude lower than the typical FR break ($L_{150} = 10^{26}$ W Hz$^{-1}$). We examine the compact features and perform spectral index analysis to identify hotspots, cores, and signatures of restarting or remnant activity. We find a higher prevalence of cores and a comparable number of hotspots in the low-luminosity FRII sample compared to a randomly selected sample of luminous ($L_{150}\gt 10^{26}$ W Hz$^{-1}$) FRIIs selected from the same parent LOFAR sample. Approximately 32 per cent of low-luminosity FRIIs show restarting or remnant behaviour, while ${\sim} 32$ per cent are active FRIIs with compact hotspots. Our results show that FRII source dynamics occur at low-radio luminosities, but reinforce earlier conclusions that the population of low-luminosity edge-brightened RLAGN is highly diverse. Binary morphological classifications should be used cautiously as a first step towards more nuanced investigations of the complexity of jet life cycles and evolution.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $3,046
Funders: National Science Foundation, Natural Resources Wales, UK Research and Innovation, University of Hertfordshire, Science Foundation Ireland, Bundesministerium für Bildung und Forschung, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Max-Planck-Gesellschaft, Ministerstwo Edukacji i Nauki, Centre National de la Recherche Scientifique, Istituto Nazionale di Astrofisica, Université d'Orléans, Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen, Gauss Centre for Supercomputing, Institut sur la Nutrition et les Aliments Fonctionnels, Observatoire de Paris, Université de Recherche Paris Sciences et Lettres, Science and Technology Facilities Council
Awards: The UK Square Kilometre Array Regional Centre 2023-2025, G1350351439, Star-forming radio galaxies: genesis, evolution, and impact, G2156317396, Astronomy at The Open University 2023-2026 (Consolidated Grant), LOFAR Data Valorization, Unveiling the physics of radio AGN feedback with LOFAR, G6544976945, LOFAR Data Valorization, LOFAR-UK 2016-2019: LOFAR-UK Compute Facility, Astronomy at the Open University 2020-2023
OpenAlex ID: W7160954258
