The prevalence of FRI radio quasars

We present deep, multi-VLA-configuration radio images for a set of 18 quasars, having redshifts between 0.36 and 2.5, from the 7C quasar survey. Approximately one quarter of these quasars have FRI-type twin-jet structures and the remainder are a broad range of wide angle tail, fat double, classical...

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Main Authors: Heywood, I, Blundell, K, Rawlings, S
Format: Journal article
Language:English
Published: 2007
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author Heywood, I
Blundell, K
Rawlings, S
author_facet Heywood, I
Blundell, K
Rawlings, S
author_sort Heywood, I
collection OXFORD
description We present deep, multi-VLA-configuration radio images for a set of 18 quasars, having redshifts between 0.36 and 2.5, from the 7C quasar survey. Approximately one quarter of these quasars have FRI-type twin-jet structures and the remainder are a broad range of wide angle tail, fat double, classical double, core-jet and hybrid sources. These images demonstrate that FRI quasars are prevalent in the universe, rather than non-existent as had been suggested in the literature prior to the serendipitous discovery of the first FRI quasar a few years ago, the optically powerful "radio quiet" quasar E1821+643. Some of the FRI quasars have radio luminosities exceeding the traditional FRI / FRII break luminosity, however we find no evidence for FRII quasars with luminosities significantly below the break. We consider whether the existence of such high luminosity FRI structures is due to the increasingly inhomogeneous environments in the higher redshift universe.
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spelling oxford-uuid:45479695-a579-455b-82ff-d241461e7bfc2022-03-26T15:06:50ZThe prevalence of FRI radio quasarsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:45479695-a579-455b-82ff-d241461e7bfcEnglishSymplectic Elements at Oxford2007Heywood, IBlundell, KRawlings, SWe present deep, multi-VLA-configuration radio images for a set of 18 quasars, having redshifts between 0.36 and 2.5, from the 7C quasar survey. Approximately one quarter of these quasars have FRI-type twin-jet structures and the remainder are a broad range of wide angle tail, fat double, classical double, core-jet and hybrid sources. These images demonstrate that FRI quasars are prevalent in the universe, rather than non-existent as had been suggested in the literature prior to the serendipitous discovery of the first FRI quasar a few years ago, the optically powerful "radio quiet" quasar E1821+643. Some of the FRI quasars have radio luminosities exceeding the traditional FRI / FRII break luminosity, however we find no evidence for FRII quasars with luminosities significantly below the break. We consider whether the existence of such high luminosity FRI structures is due to the increasingly inhomogeneous environments in the higher redshift universe.
spellingShingle Heywood, I
Blundell, K
Rawlings, S
The prevalence of FRI radio quasars
title The prevalence of FRI radio quasars
title_full The prevalence of FRI radio quasars
title_fullStr The prevalence of FRI radio quasars
title_full_unstemmed The prevalence of FRI radio quasars
title_short The prevalence of FRI radio quasars
title_sort prevalence of fri radio quasars
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