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dc.contributor.authorWorrall, D.M.
dc.contributor.authorBirkinshaw, M.
dc.contributor.authorHardcastle, M.J.
dc.date.accessioned2008-02-01T11:34:59Z
dc.date.available2008-02-01T11:34:59Z
dc.date.issued2001
dc.identifier.citationWorrall , D M , Birkinshaw , M & Hardcastle , M J 2001 , New radio-galaxy X-ray results from Chandra . in In: Procs of Particles and Fields in Radio Galaxies Conference, ASP Conference Proceedings 250 . Astronomical Society of the Pacific , pp. 224-229 .
dc.identifier.isbn1-58381-090-0
dc.identifier.otherPURE: 178252
dc.identifier.otherPURE UUID: 8c883e54-16b5-4663-9e85-d9f60f3b4201
dc.identifier.otherdspace: 2299/1505
dc.identifier.urihttp://hdl.handle.net/2299/1505
dc.description.abstractThe superior spatial resolution of the Chandra X-ray Observatory is sharpening our X-ray vision of extragalactic radio sources. Our recent Guest Observer observations of a small sample of B2 radio galaxies show jet X-ray emission to be common in low-power radio galaxies, whereas previously such jets were only X-ray detected in nearby Cen A and M 87. At high redshift, Chandra clearly separates AGN-related emission from the surrounding X-ray emitting cluster medium, as illustrated by our results for 3C 220.1 at a redshift of 0.6.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Particles and Fields in Radio Galaxies Conference, ASP Conference Proceedings 250
dc.titleNew radio-galaxy X-ray results from Chandraen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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