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dc.contributor.authorBouy, H.
dc.contributor.authorGirard, J.H.V.
dc.contributor.authorMartin, E.L.
dc.contributor.authorHuelamo, N.
dc.contributor.authorLucas, P.W.
dc.date.accessioned2011-12-19T16:01:39Z
dc.date.available2011-12-19T16:01:39Z
dc.date.issued2011
dc.identifier.citationBouy , H , Girard , J H V , Martin , E L , Huelamo , N & Lucas , P W 2011 , ' Adaptive optics observations of the T10 ultracool dwarf UGPS J072227.51-054031.2 ' , Astronomy and Astrophysics , vol. 526 , no. 7 . https://doi.org/10.1051/0004-6361/201015289
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 182232
dc.identifier.otherPURE UUID: 208bcf2e-11f1-4d4d-b655-38a51cac929b
dc.identifier.otherdspace: 2299/5217
dc.identifier.otherScopus: 78650459038
dc.identifier.otherORCID: /0000-0002-8872-4462/work/62748909
dc.identifier.urihttp://hdl.handle.net/2299/7365
dc.descriptionOriginal article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory
dc.description.abstractContext: With a spectral type of T10, UGPS J072227.51-054031.2 is one of the coolest objects known to date in the solar neighborhood. Aims: Multiple systems are relatively common among early and mid-T dwarfs. We search for faint and close companions around UGPS J072227.51-054031.2. Methods: We have obtained high spatial resolution images in the H and Ks bands using adaptive optics at the Very Large Telescope. Results: With a Strehl ratio in the range 10–15%, the final images allow us to rule out the presence of a companion brighter than H 19.4 mag at separation larger than 50 mas, and H 21.4 mag at separation larger than 01.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectBinaries: general
dc.subjectbrown dwarfs
dc.subjecttechniques: high angular resolution
dc.titleAdaptive optics observations of the T10 ultracool dwarf UGPS J072227.51-054031.2en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361/201015289
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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