Radio-loud AGN: is there a link between luminosity and cluster environment?
arXiv:1305.1050 · doi:10.1088/0004-637X/770/2/136
Abstract
We present here the first results from the Chandra ERA (Environments of Radio-loud AGN) Large Project, characterizing the cluster environments of a sample of 26 radio-loud AGN at z ~ 0.5 that covers three decades of radio luminosity. This is the first systematic X-ray environmental study at a single epoch, and has allowed us to examine the relationship between radio luminosity and cluster environment without the problems of Malmquist bias. We have found a weak correlation between radio luminosity and host cluster X-ray luminosity, as well as tentative evidence that this correlation is driven by the subpopulation of low-excitation radio galaxies, with high-excitation radio galaxies showing no significant correlation. The considerable scatter in the environments may be indicative of complex relationships not currently included in feedback models.
Accepted for publication in ApJ, 16 pages, 12 figures, 7 tables
References in corpus (10)
- Heating Hot Atmospheres with Active Galactic Nuclei
- Hot and cold gas accretion and feedback in radio-loud active galaxies
- Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
- The X-ray nuclei of intermediate-redshift radio sources
- Spitzer Reveals Hidden Quasar Nuclei in Some Powerful FR II Radio Galaxies
- Tracing the evolution in the iron content of the ICM
- High-energy particle acceleration at the radio-lobe shock of Centaurus A
- An XMM-Newton study of the environments, particle content and impact of low-power radio galaxies
- Observed properties of FRII quasars and radio galaxies at z < 1.0
- High redshift FRII radio sources: large-scale X-ray environment
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