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dc.contributor.authorHardcastle, M.J.
dc.contributor.authorAlexander, P.
dc.contributor.authorPooley, G.G.
dc.contributor.authorRiley, J.M.
dc.date.accessioned2007-12-17T09:54:27Z
dc.date.available2007-12-17T09:54:27Z
dc.date.issued1999
dc.identifier.citationHardcastle , M J , Alexander , P , Pooley , G G & Riley , J M 1999 , ' FR II radio galaxies with z <0.3 -- II. Beaming and unification ' , Monthly Notices of the Royal Astronomical Society , vol. 304 , no. 1 , pp. 135-144 . https://doi.org/10.1046/j.1365-8711.1999.02298.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 158599
dc.identifier.otherPURE UUID: 197d8e9a-8b5c-4f52-8b90-615e103f2ab6
dc.identifier.otherdspace: 2299/1197
dc.identifier.otherScopus: 0041708491
dc.identifier.urihttp://hdl.handle.net/2299/1197
dc.descriptionThe definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing --DOI : 10.1046/j.1365-8711.1999.02298.x
dc.description.abstractIn a previous paper we presented measurements of the properties of jets and cores in a large sample of FRII radio galaxies with z < 0.3. Here we test, by means of Monte Carlo simulations, the consistency of those data with models in which the prominences of cores and jets are determined by relativistic beaming. We conclude that relativistic beaming is needed to explain the relationships between core and jet prominences, and that speeds between 0.5 and 0.7c on kpc scales provide the best fits to the data.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleFR II radio galaxies with z<0.3 -- II. Beaming and unificationen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1046/j.1365-8711.1999.02298.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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