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dc.contributor.authorGiles, A.B.
dc.contributor.authorKing, A.R.
dc.contributor.authorJameson, R.F.
dc.contributor.authorSherrington, M.R.
dc.contributor.authorHough, J.
dc.contributor.authorBailey, J.
dc.contributor.authorCunningham, E.C.
dc.date.accessioned2009-04-22T09:10:05Z
dc.date.available2009-04-22T09:10:05Z
dc.date.issued1980
dc.identifier.citationGiles , A B , King , A R , Jameson , R F , Sherrington , M R , Hough , J , Bailey , J & Cunningham , E C 1980 , ' The IR variability of SS433 ' , Nature , vol. 286 , no. 5774 , pp. 689-691 . https://doi.org/10.1038/286689a0
dc.identifier.issn0028-0836
dc.identifier.otherPURE: 170492
dc.identifier.otherPURE UUID: 68d8cd2f-7e3f-44e7-a3b1-063b2ed9b622
dc.identifier.otherdspace: 2299/3263
dc.identifier.otherScopus: 0040956802
dc.identifier.urihttp://hdl.handle.net/2299/3263
dc.descriptionOriginal article can be found at: http://www.nature.com/nature/ Copyright Nature Publishing Group. DOI: 10.1038/286689a0 [Full text of this article is not available in the UHRA]
dc.description.abstractWe report here the results of a one-year monitoring programme of SS433 at IR and visual wavelengths. The most striking feature of these observations is the near constancy of the IR colours while the source's flux varies over a range of 1.2 mag. There is no evidence for the 13.1-day period first reported in radial-velocity measurements by Crampton et al. However, it seems possible that an 11.8-day period is present.en
dc.language.isoeng
dc.relation.ispartofNature
dc.titleThe IR variability of SS433en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1980
rioxxterms.versionofrecordhttps://doi.org/10.1038/286689a0
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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