University of Hertfordshire

From the same journal

From the same journal

By the same authors

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

Research output: Contribution to journalArticle

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    Accepted author manuscript, 859 KB, PDF document

  • 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
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Original languageEnglish
Pages (from-to)280-289
JournalMonthly Notices of the Royal Astronomical Society
Volume445
Issue1
Early online date24 Sep 2014
DOIs
Publication statusPublished - 21 Nov 2014

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

Notes

Date of Acceptance: 20/08/2014

ID: 9226756