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19982022
most citedDistant Radio Galaxies and their Environments

418 citations · 3.5k across the 49 of their papers we have counts for

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Showing 2008Show all

7 papers · 1 filter

astro-ph20084 cited

Gas and Stars in Galaxies - A Multi-Wavelength 3D Perspective

Matt Lehnert, Carlos De Breuck, Harald Kuntschner +1

An overview of the ESO/Radionet workshop devoted to 3D optical/near-infrared and sub-mm/radio observations of gas and stars in galaxies is presented. There will be no published pro…

astro-ph2008326 cited

Evidence for powerful AGN winds at high redshift: Dynamics of galactic outflows in radio galaxies during the "Quasar Era"

N. P. H. Nesvadba, M. D. Lehnert, C. De Breuck +2

AGN feedback now appears as an attractive mechanism to resolve some of the outstanding problems with the "standard" cosmological models, in particular those related to massive gala…

astro-ph20087 cited

Spatially extended absorption around the z=2.63 radio galaxy MRC 2025-218: outflow or infall?

A. Humphrey, M. Villar-Martin, S. F. Sanchez +7

We present an investigation into the absorber in front of the z=2.63 radio galaxy MRC 2025-218, using integral field spectroscopy obtained at the Very Large Telescope, and long sli…

astro-ph200830 cited

Mid-Infrared Spectra of High Redshift (z>2) Radio Galaxies

N. Seymour, P. Ogle, C. De Breuck +8

We present the first mid-infrared Spitzer/Infrared Spectrograph (IRS) observations of powerful radio galaxies at z>2. These radio galaxies, 4C +23.56 (z=2.48) and 6C J1908+7220 (z=…

astro-ph200834 cited

Submillimeter observations of the J2142-4423 Lya protocluster at z = 2.38

A. Beelen, A. Omont, N. Bavouzet +9

We present observations aimed at exploring both the nature of Lya emitting nebulae (Lya blobs) at z=2.38 and the way they trace large scale structure (LSS), by exploring their prox…

astro-ph2008418 cited

Distant Radio Galaxies and their Environments

George Miley, Carlos De Breuck

We review the properties and nature of luminous high-redshift radio galaxies (HzRGs, z > 2) and the environments in which they are located. HzRGs have several distinct constituents…