Research output: Contribution to journal › Article › peer-review
- 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
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