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dc.contributor.authorBarnes, J.R.
dc.contributor.authorBarman, T.S.
dc.contributor.authorPrato, L.
dc.contributor.authorSegransan, D.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorLeigh, C.J.
dc.contributor.authorCollier Cameron, A.
dc.contributor.authorPinfield, D.J.
dc.date.accessioned2008-07-21T08:31:08Z
dc.date.available2008-07-21T08:31:08Z
dc.date.issued2007
dc.identifier.citationBarnes , J R , Barman , T S , Prato , L , Segransan , D , Jones , H R A , Leigh , C J , Collier Cameron , A & Pinfield , D J 2007 , ' Limits on the 2.2- m contrast ratio of the close-orbiting planet HD 189733b ' , Monthly Notices of the Royal Astronomical Society , vol. 382 , no. 1 , pp. 473-480 . https://doi.org/10.1111/j.1365-2966.2007.12394.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 167360
dc.identifier.otherPURE UUID: dc985692-b6f8-4932-9a35-6e17cf1527eb
dc.identifier.otherdspace: 2299/2230
dc.identifier.otherScopus: 36148983098
dc.identifier.urihttp://hdl.handle.net/2299/2230
dc.descriptionThe definitive version is available at: www.blackwell-synergy.com. Copyright Balckwell Publishing DOI : 10.1111/j.1365-2966.2007.12394.x
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleLimits on the 2.2- m contrast ratio of the close-orbiting planet HD 189733ben
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2007.12394.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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