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

Centre for Astrophysics Research (CAR)

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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 language	English
Pages (from-to)	280-289
Journal	Monthly Notices of the Royal Astronomical Society
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 10^14 solar mass cluster having experienced powerful radio-loud feedback of duration ~60 Myr during 1.3",

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doi = "10.1093/mnras/stu1725",

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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

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

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

Abstract

Keywords

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