The large-scale environment of FR 0 radio galaxies
arXiv:2009.03330 · doi:10.1051/0004-6361/201935962
Abstract
We explore the properties of the large-scale environment of FR0 radio galaxies belonging to the FR0CAT sample which includes 104 compact radio sources associated with nearby (z<0.05) early-type galaxies. By using various estimators we find that FR0s live in regions of higher than the average galaxies density and a factor two lower density, on average, with respect to FRI radio galaxies. This latter difference is driven by the large fraction (63%) of FR0s located in groups formed by less than 15 galaxies, an environment which FRIs rarely (17%) inhabit. Beside the lack of substantial extended radio emission defining the FR0s class, this is the first significant difference between the properties of these two populations of low power radio galaxies. We interpret the differences in environment between FR0s and FRIs as the due to an evolutionary link between local galaxies density, BH spin, jet power, and extended radio emission.
arXiv comment11 pages, 6 figures, 3 tables (Pre-proofs version - Published in A&A)
References in corpus (31)
- LOFAR: The LOw-Frequency ARray
- The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
- On the fundamental dichotomy in the local radio-AGN population: accretion, evolution, and host galaxy properties
- Black Hole Spin and the Radio Loud/Quiet Dichotomy of Active Galactic Nuclei
- The relation between accretion rate and jet power in X-ray luminous elliptical galaxies
- The 1% Concordance Hubble Constant
- Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue
- The Last of FIRST: The Final Catalog and Source Identifications
- A sample of radio-loud AGN in the Sloan Digital Sky Survey
- Total and Jet Blandford-Znajek Power in Presence of Accretion Disk
- Black hole evolution: III. Statistical properties of mass growth and spin evolution using large-scale hydrodynamical cosmological simulations
- A pilot study of the radio-emitting AGN population: the emerging new class of FR0 radio-galaxies
- Groups and clusters of galaxies in the SDSS DR8. Value-added catalogues
- FR II radio galaxies with z<0.3 -- I. Properties of jets, cores and hot spots
- The accretion mechanism in low-power radio galaxies
- The environmental dependence of radio-loud AGN activity and star formation in the 2dFGRS
- The local radio-galaxy population at 20 GHz
- FR0CAT: a FIRST catalog of FR0 radio galaxies
- The relation between morphology, accretion modes and environmental factors in local radio AGN
- Galaxy morphology, luminosity and, environment in the SDSS DR7
- FRICAT: A FIRST catalog of FRI radio galaxies
- High-resolution VLA observations of FR0 radio galaxies: properties and nature of compact radio sources
- Radio and spectroscopic properties of miniature radio galaxies: revealing the bulk of the radio-loud AGN population
- The environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS)
- What governs the bulk velocity of the jet components in active galactic nuclei?
- X-ray study of a sample of FR0 radio galaxies: unveiling the nature of the central engine
- Parsec-scale radio structure of 14 Fanaroff-Riley type 0 radio galaxies
- FR0 radio galaxies and their place in the radio morphology classification
- Deciphering the large-scale environment of radio galaxies in the local Universe: where do they born, grow and die?
- The XXL survey XXXV. The role of cluster mass in AGN activity
- Accretion and nuclear activity in Virgo early-type galaxies
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- Compact steep-spectrum and peaked-spectrum radio sources
- A population of galaxy-scale jets discovered using LOFAR
- The LOFAR view of FR0 radio galaxies
- Scrutinizing FR 0 Radio Galaxies as Ultra-High-Energy Cosmic Ray Source Candidates
- Jet-accretion system in the nearby mJy Radio Galaxies
- Characterising the extended morphologies of BL Lacs at 144 MHz with LOFAR
- The LOFAR view of massive early-type galaxies: Transition from radio AGN to host emission
- The central FR0 in the sloshing cluster Abell 795: Indications of mechanical feedback from Chandra data
- Is jet re-orientation the elusive trigger for star formation suppression in radio galaxies?
- The emergence of the X-ray luminosity/cluster richness relation for radio galaxies
- The eMERLIN and EVN view of FR0 radio galaxies