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dc.contributor.authorLucas, P.W.
dc.contributor.authorHough, J.
dc.contributor.authorBailey, J.
dc.contributor.authorTamura, M.
dc.contributor.authorHirst, E.
dc.contributor.authorHarrison, D.
dc.date.accessioned2013-01-07T09:29:15Z
dc.date.available2013-01-07T09:29:15Z
dc.date.issued2009
dc.identifier.citationLucas , P W , Hough , J , Bailey , J , Tamura , M , Hirst , E & Harrison , D 2009 , ' Planetpol polarimetry of the exoplanet systems 55 Cnc and tau Boo ' , Monthly Notices of the Royal Astronomical Society , vol. 393 , no. 1 , pp. 229-244 . https://doi.org/10.1111/j.1365-2966.2008.14182.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 169488
dc.identifier.otherPURE UUID: dae60a49-c372-4df1-9fb4-2141b7bac91a
dc.identifier.otherdspace: 2299/3440
dc.identifier.otherScopus: 58649124745
dc.identifier.otherORCID: /0000-0002-8872-4462/work/62748886
dc.identifier.urihttp://hdl.handle.net/2299/9483
dc.description‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing / Royal Astronomical Society
dc.description.abstractWe present very sensitive polarimetry of 55 Cnc and τ Boo in an attempt to detect the partially polarized reflected light from the planets orbiting these two stars. 55 Cnc is orbited by a hot Neptune planet (55 Cnc e) at 0.038 au, a hot Jupiter planet (55 Cnc b) at 0.11 au and at least three more distant planets. The polarization of this system is very stable, showing no sign of the periodic variations that would be expected if a short-period planet were detected.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titlePlanetpol polarimetry of the exoplanet systems 55 Cnc and tau Booen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionParticle Instruments and diagnostics
dc.description.statusPeer reviewed
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2008.14182.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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