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dc.contributor.authorEvans, D.A.
dc.contributor.authorHardcastle, M.J.
dc.contributor.authorLee, J.C.
dc.contributor.authorKraft, R.P.
dc.contributor.authorWorrall, D.M.
dc.contributor.authorBirkinshaw, M.
dc.contributor.authorCroston, J.H.
dc.date.accessioned2008-12-17T09:18:19Z
dc.date.available2008-12-17T09:18:19Z
dc.date.issued2008
dc.identifier.citationEvans , D A , Hardcastle , M J , Lee , J C , Kraft , R P , Worrall , D M , Birkinshaw , M & Croston , J H 2008 , ' XMM-Newton Observations of the Nuclei of the Radio Galaxies 3C 305, DA 240, and 4C 73.08 ' , The Astrophysical Journal , vol. 688 , no. 2 , pp. 844-851 . https://doi.org/10.1086/592266
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 148287
dc.identifier.otherPURE UUID: 72150117-9c8b-411b-9889-2f1601e907db
dc.identifier.otherdspace: 2299/2699
dc.identifier.otherScopus: 56849121266
dc.identifier.urihttp://hdl.handle.net/2299/2699
dc.descriptionOriginal article can be found at: http://www.journals.uchicago.edu/loi/ApJ/ Copyright American Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractWe present new XMM-Newton EPIC observations of the nuclei of the nearby radio galaxies 3C 305, DA 240, and 4C 73.08, and investigate the origin of their nuclear X-ray emission. The nuclei of the three sources appear to have different relative contributions of accretion- and jet-related X-ray emission, as expected based on earlier work. The X-ray spectrum of the FR II narrow-line radio galaxy (NLRG) 4C 73.08 is modeled with the sum of a heavily absorbed power law that we interpret to be associated with a luminous accretion disk and circumnuclear obscuring structure, and an unabsorbed power law that originates in an unresolved jet. This behavior is consistent with other narrow-line radio galaxies. The X-ray emission of the low-excitation FR II radio galaxy DA 240 is best modeled as an unabsorbed power law that we associate with a parsec-scale jet, similar to other low-excitation sources that we have studied previously. However, the X-ray nucleus of the narrow-line radio galaxy 3C 305 shows no evidence for the heavily absorbed X-ray emission that has been found in other NLRGs. It is possible that the nuclear optical spectrum in 3C 305 is intrinsically weak-lined, with the strong emission arising from extended regions that indicate the presence of jet-environment interactions. Our observations of 3C 305 suggest that this source is more closely related to other weak-lined radio galaxies. This ambiguity could extend to other sources currently classified as NLRGs. We also present XMM-Newton and VLA observations of the hot spot of DA 240, arguing that this is another detection of X-ray synchrotron emission from a low-luminosity hot spot.en
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleXMM-Newton Observations of the Nuclei of the Radio Galaxies 3C 305, DA 240, and 4C 73.08en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2008
rioxxterms.versionofrecordhttps://doi.org/10.1086/592266
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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