The environment of radio galaxies: a signature of AGN feedback at high redshifts
- 20 July 2018
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 480 (1) , 1340-1352
Abstract
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Funding Information
- Science and Technology Facilities Council (ST/L00075X/1, ST/P000451/1, ST/K00042X/1, ST/H008519/1, ST/K00087X/1, ST/K003267/1)
This publication has 95 references indexed in Scilit:
- Radio Jets Clearing the Way Through a Galaxy: Watching Feedback in ActionScience, 2013
- STRONG MOLECULAR HYDROGEN EMISSION AND KINEMATICS OF THE MULTIPHASE GAS IN RADIO GALAXIES WITH FAST JET-DRIVEN OUTFLOWSThe Astrophysical Journal, 2012
- INTRACLUSTER MEDIUM REHEATING BY RELATIVISTIC JETSThe Astrophysical Journal, 2011
- RELATIVISTIC JET FEEDBACK IN EVOLVING GALAXIESThe Astrophysical Journal, 2011
- Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z 0.5Monthly Notices of the Royal Astronomical Society, 2007
- On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flowsMonthly Notices of the Royal Astronomical Society, 2007
- The UKIRT Infrared Deep Sky Survey (UKIDSS)Monthly Notices of the Royal Astronomical Society, 2007
- Accretion, feedback and galaxy bimodality: a comparison of the GalICS semi-analytic model and cosmological SPH simulationsMonthly Notices of the Royal Astronomical Society, 2007
- Breaking the hierarchy of galaxy formationMonthly Notices of the Royal Astronomical Society, 2006
- Grand unification of AGN and the accretion and spin paradigmsNew Astronomy Reviews, 2002