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dc.contributor.authorHawkins, M.R.S.
dc.contributor.authorDucourant, C.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorRapaport, M.
dc.date.accessioned2008-02-01T11:43:58Z
dc.date.available2008-02-01T11:43:58Z
dc.date.issued1998
dc.identifier.citationHawkins , M R S , Ducourant , C , Jones , H R A & Rapaport , M 1998 , A New Population of Brown Dwarfs . in In: Brown Dwarfs and Extrasolar Planets - ASP Conf Series 134 . Astronomical Society of the Pacific , pp. 106-8 .
dc.identifier.isbn1-886733-54-6
dc.identifier.otherPURE: 142771
dc.identifier.otherPURE UUID: 566a329f-8cbf-49ea-9dbe-5edb77bdd483
dc.identifier.otherdspace: 2299/1527
dc.identifier.otherScopus: 0000752391
dc.identifier.urihttp://hdl.handle.net/2299/1527
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/113-155.html--Copyright Astronomical Society of the Pacific
dc.description.abstractA large area deep survey for brown dwarfs from digitally stacked 1.2m Schmidt plates has revealed a population of very red stars (R-I>3). On the basis of their colours, near IR spectra and their luminosity estimates from proper motions, these objects appeared to be Brown Dwarfs. First measurements of the parallaxes of 8 of the reddest objects at the 1.5 danish telescope confirmed this, and showed that four of them have K-band luminosities some mags below the bottom of the main sequence. We present here those results.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Brown Dwarfs and Extrasolar Planets - ASP Conf Series 134
dc.rightsOpen
dc.titleA New Population of Brown Dwarfsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1998
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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