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dc.contributor.authorHardcastle, M.J.
dc.contributor.authorKrause, Martin
dc.date.accessioned2014-08-12T09:30:42Z
dc.date.available2014-08-12T09:30:42Z
dc.date.issued2014-09-11
dc.identifier.citationHardcastle , M J & Krause , M 2014 , ' Numerical modelling of the lobes of radio galaxies in cluster environments II : Magnetic field configuration and observability ' , Monthly Notices of the Royal Astronomical Society , vol. 443 , pp. 1482-1499 . https://doi.org/10.1093/mnras/stu1229
dc.identifier.issn1365-2966
dc.identifier.otherPURE: 7227050
dc.identifier.otherPURE UUID: f404b544-4573-4453-86e9-3f1f9d0d845b
dc.identifier.otherArXiv: http://arxiv.org/abs/1406.5300v1
dc.identifier.otherScopus: 84905656800
dc.identifier.urihttp://hdl.handle.net/2299/14336
dc.descriptionCopyright The Authors 2014. Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstractWe describe three-dimensional magnetohydrodynamical modelling of powerful radio galaxies in realistic poor cluster environments. This modelling extends our earlier work on the hydrodynamics of radio galaxies as a function of their cluster environment to consider the magnetic field configuration in the lobes and its observational consequences, using a realistic model for the magnetic field in the intracluster medium, very high density contrast in the lobes and high numerical resolution. We confirm, now with a realistic magnetic field model, that lobes have characteristic trajectories in the radio power/linear size diagram which depend strongly on their environment. We investigate the detailed evolution of polarized emission, showing that the lobes evolve from the initially ordered field configuration imposed by our boundary conditions to one in which the longitudinal field comes to dominate. We obtain simulated observations of polarization whose properties are quantitatively consistent with observations. The highly spatially intermittent magnetic field also reproduces the observation that inverse-Compton emission from lobes is much smoother than synchrotron. Our simulations allow us to study the depolarizing effect of the external medium on the lobes, and so to demonstrate that Faraday depolarization from environments of the type we consider can reproduce the integrated fractional polarization properties of large samples and the observed preferential depolarization of the receding lobe.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rights/dk/atira/pure/core/openaccesspermission/open
dc.subjectastro-ph.HE
dc.subjectastro-ph.GA
dc.titleNumerical modelling of the lobes of radio galaxies in cluster environments II : Magnetic field configuration and observabilityen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2014-06-19
rioxxterms.versionSMUR
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stu1229
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeopenAccess


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