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

doi:10.1093/mnras/stu1725

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 journal › Article › peer-review

99 Citations (Scopus)

192 Downloads (Pure)

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 language	English
Pages (from-to)	280-289
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	445
Issue number	1
Early online date	24 Sept 2014
DOIs	https://doi.org/10.1093/mnras/stu1725
Publication status	Published - 21 Nov 2014

Keywords

astro-ph.GA
astro-ph.CO

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title = "Why z > 1 radio-loud galaxies are commonly located in protoclusters",

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\textasciicircum{}14 solar mass cluster having experienced powerful radio-loud feedback of duration \textasciitilde{}60 Myr during 1.3",

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doi = "10.1093/mnras/stu1725",

language = "English",

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T1 - Why z > 1 radio-loud galaxies are commonly located in protoclusters

AU - Hatch, N. A.

AU - Wylezalek, D.

AU - Kurk, J. D.

AU - Stern, D.

AU - Breuck, C. De

AU - Jarvis, M.J.

AU - Galametz, A.

AU - Gonzalez, A. H.

AU - Hartley, W. G.

AU - Mortlock, A.

AU - Seymour, N.

AU - Stevens, J. A.

N1 - Date of Acceptance: 20/08/2014

PY - 2014/11/21

Y1 - 2014/11/21

N2 - 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

AB - 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

KW - astro-ph.GA

KW - astro-ph.CO

U2 - 10.1093/mnras/stu1725

DO - 10.1093/mnras/stu1725

M3 - Article

SN - 0035-8711

VL - 445

SP - 280

EP - 289

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

IS - 1

ER -

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

Abstract

Keywords

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