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dc.contributor.authorBrindle, C.
dc.contributor.authorHough, J.
dc.contributor.authorBailey, J.
dc.contributor.authorAxon, D.J.
dc.contributor.authorSchulz, H.
dc.contributor.authorKikuchi, S.
dc.contributor.authorMcGraw, J.T.
dc.contributor.authorWisniewski, W.J.
dc.contributor.authorFontaine, J.
dc.contributor.authorNadesu, D.
dc.contributor.authorClayton, G.
dc.contributor.authorAnderson, E.
dc.contributor.authorJameson, R.F.
dc.contributor.authorNadesu, D.
dc.contributor.authorClayton, G.
dc.contributor.authorAnderson, E.
dc.contributor.authorJameson, R.F.
dc.contributor.authorSmith, R.
dc.contributor.authorWallis, R.E.
dc.date.accessioned2009-04-21T12:25:29Z
dc.date.available2009-04-21T12:25:29Z
dc.date.issued1985
dc.identifier.citationBrindle , C , Hough , J , Bailey , J , Axon , D J , Schulz , H , Kikuchi , S , McGraw , J T , Wisniewski , W J , Fontaine , J , Nadesu , D , Clayton , G , Anderson , E , Jameson , R F , Nadesu , D , Clayton , G , Anderson , E , Jameson , R F , Smith , R & Wallis , R E 1985 , ' Coordinated multisite observations of the variability of BL Lac ' , Monthly Notices of the Royal Astronomical Society , vol. 214 , no. 4 , pp. 619-638 . < http://cdsads.u-strasbg.fr/ >
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 165043
dc.identifier.otherPURE UUID: 6f8a7cbb-90a3-4401-9ac2-c9f44aa625b7
dc.identifier.otherdspace: 2299/3249
dc.identifier.urihttp://hdl.handle.net/2299/3249
dc.descriptionOriginal article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractThe authors present the results of multisite observations of the optical polarization of BL Lac, together with some flux measurements, at a time when BL Lac was relatively faint. The level of polarization varies in a manner similar to that reported by Moore et al., although the position angle behaviour is quite different, varying only a small amount from a mean of 28°. Models are presented to account for the observed polarization behaviour of BL Lac. The best model is one consisting of two polarized components, one having a variable polarization, intensity and random position angle, and the other a fixed polarization, intensity and position angle. The authors tentatively identify this latter component as being associated with the inner region of the optical jet of BL Lac.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleCoordinated multisite observations of the variability of BL Lacen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://cdsads.u-strasbg.fr/
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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