Why z > 1 radio-loud galaxies are commonly located in protoclusters

N. A. Hatch, D. Wylezalek, J. D. Kurk, D. Stern, C. De Breuck, M.J. Jarvis, A. Galametz, A. H. Gonzalez, W. G. Hartley, A. Mortlock, N. Seymour, J. A. Stevens

Research output: Contribution to journalArticlepeer-review

56 Citations (Scopus)
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Abstract

Distant powerful radio-loud active galactic nuclei (RLAGN) tend to reside in dense environments and are commonly found in proto-clusters at z > 1.3. We examine whether this occurs because RLAGN are hosted by massive galaxies, which preferentially reside in rich environments. We compare the environments of powerful RLAGN at 1.3 10^14 solar mass cluster having experienced powerful radio-loud feedback of duration ~60 Myr during 1.3
Original languageEnglish
Pages (from-to)280-289
JournalMonthly Notices of the Royal Astronomical Society
Volume445
Issue number1
Early online date24 Sept 2014
DOIs
Publication statusPublished - 21 Nov 2014

Keywords

  • astro-ph.GA
  • astro-ph.CO

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