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dc.contributor.authorHardcastle, M.J.
dc.contributor.authorWorrall, D.M.
dc.date.accessioned2007-12-17T09:51:39Z
dc.date.available2007-12-17T09:51:39Z
dc.date.issued2000
dc.identifier.citationHardcastle , M J & Worrall , D M 2000 , ' Radio, optical and X-ray nuclei in nearby 3CRR radio galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 314 , no. 2 , pp. 359363 . https://doi.org/10.1046/j.1365-8711.2000.03393.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 137799
dc.identifier.otherPURE UUID: 54aace94-7c78-4c6c-b9a0-95f5de3ded20
dc.identifier.otherdspace: 2299/1192
dc.identifier.otherScopus: 0000542782
dc.identifier.urihttp://hdl.handle.net/2299/1192
dc.descriptionThe definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI : 10.1046/j.1365-8711.2000.03393.x
dc.description.abstractHST observations have shown that low-redshift 3CR radio galaxies often exhibit a point-like optical component positionally coincident with the GHz-frequency radio core. In this paper we discuss the correlation between the luminosities of the radio, optical and X-ray cores in these objects, and argue that all three components have a common origin at the base of the relativistic jets. In unified models, FRI radio galaxies should appear as dimmed, redshifted versions of BL Lac objects. We show that such models are consistent with the spectral energy distributions of the radio galaxies only if the nuclear X-ray emission in radio galaxies is inverse-Compton in origin.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleRadio, optical and X-ray nuclei in nearby 3CRR radio galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1046/j.1365-8711.2000.03393.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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