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dc.contributor.authorHardcastle, M.J.
dc.date.accessioned2007-12-17T09:54:28Z
dc.date.available2007-12-17T09:54:28Z
dc.date.issued1998
dc.identifier.citationHardcastle , M J 1998 , ' Jets, plumes and hotspots in the wide-angle tail source 3C 130 ' , Monthly Notices of the Royal Astronomical Society , vol. 298 , no. 2 , pp. 569-576 . https://doi.org/10.1046/j.1365-8711.1998.01662.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 145141
dc.identifier.otherPURE UUID: 39b633e1-b711-4f38-9fac-6757841c374f
dc.identifier.otherdspace: 2299/1198
dc.identifier.otherScopus: 1542389388
dc.identifier.urihttp://hdl.handle.net/2299/1198
dc.descriptionThe definitive version is available at www.blackwell-synergy.com. Copyright Blackwell Publishing DOI : 10.1046/j.1365-8711.1998.01662.x
dc.description.abstractI present 1.5- and 8.4-GHz observations with all configurations of the NRAO VLA of the wide-angle tail source 3C130. The source has a pair of relatively symmetrical, well- collimated inner jets, one of which terminates in a compact hot spot. Archival ROSAT PSPC data confirm that 3C130’s environment is a luminous cluster with little sign of sub-structure in the X-ray-emitting plasma. I compare the source to other wide-angle tail objects and discuss the properties of the class as a whole. None of the currently popular models is entirely satisfactory in accounting for the disruption of the jets in 3C130.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleJets, plumes and hotspots in the wide-angle tail source 3C 130en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1046/j.1365-8711.1998.01662.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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