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

Hatch, N. A., Wylezalek, D., Kurk, J. D., Stern, D., Breuck, C. De, Jarvis, M.J., Galametz, A., Gonzalez, A. H., Hartley, W. G., Mortlock, A., Seymour, N. and Stevens, J. A. (2014) Why z > 1 radio-loud galaxies are commonly located in protoclusters. pp. 280-289. ISSN 0035-8711

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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

Item Type	Article
Uncontrolled Keywords	astro-ph.GA; astro-ph.CO
Divisions	?? sbu_spam ?? ?? ri_st ??
Date Deposited	18 Nov 2024 11:51
Last Modified	18 Nov 2024 11:51

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