University of Hertfordshire

From the same journal

From the same journal

By the same authors

Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power

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Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume471
Issue1
Early online date1 Jun 2017
DOIs
Publication statusPublished - 11 Oct 2017

Abstract

Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9z

Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2017 The Author (s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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