| dc.contributor.author | Hatch, N. A. | |
| dc.contributor.author | Wylezalek, D. | |
| dc.contributor.author | Kurk, J. D. | |
| dc.contributor.author | Stern, D. | |
| dc.contributor.author | Breuck, C. De | |
| dc.contributor.author | Jarvis, M.J. | |
| dc.contributor.author | Galametz, A. | |
| dc.contributor.author | Gonzalez, A. H. | |
| dc.contributor.author | Hartley, W. G. | |
| dc.contributor.author | Mortlock, A. | |
| dc.contributor.author | Seymour, N. | |
| dc.contributor.author | Stevens, J. A. | |
| dc.date.accessioned | 2015-09-28T14:28:49Z | |
| dc.date.available | 2015-09-28T14:28:49Z | |
| dc.date.issued | 2014-11-21 | |
| dc.identifier.citation | Hatch , N A , Wylezalek , D , Kurk , J D , Stern , D , Breuck , C D , Jarvis , M J , Galametz , A , Gonzalez , A H , Hartley , W G , Mortlock , A , Seymour , N & Stevens , J A 2014 , ' Why z > 1 radio-loud galaxies are commonly located in protoclusters ' , Monthly Notices of the Royal Astronomical Society , vol. 445 , no. 1 , pp. 280-289 . https://doi.org/10.1093/mnras/stu1725 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | ArXiv: http://arxiv.org/abs/1409.1218v1 | |
| dc.identifier.other | ORCID: /0000-0002-4010-8310/work/62747542 | |
| dc.identifier.uri | http://hdl.handle.net/2299/16461 | |
| dc.description | Date of Acceptance: 20/08/2014 | |
| dc.description.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 | en |
| dc.format.extent | 880099 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.subject | astro-ph.GA | |
| dc.subject | astro-ph.CO | |
| dc.title | Why z > 1 radio-loud galaxies are commonly located in protoclusters | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Science & Technology Research Institute | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.1093/mnras/stu1725 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
