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

Research output: Contribution to journal › Article

Documents

  • stx1333

    Final published version, 5.62 MB, PDF document

View graph of relations
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.

Projects

ID: 11938367