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dc.contributor.authorSAHLMANN, J.
dc.contributor.authorBURGASSER, A. J.
dc.contributor.authorBARDALEZ GAGLIUFFI, D. C.
dc.contributor.authorLAZORENKO, P. F.
dc.contributor.authorSÉGRANSAN, D.
dc.contributor.authorZAPATERO OSORIO, M. R.
dc.contributor.authorBLAKE, C. H.
dc.contributor.authorGELINO, C. R.
dc.contributor.authorMARTÍN, E. L.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBOUY, H.
dc.date.issued2020
dc.identifier.issn0035-8711
dc.description.abstractEnNear-infrared spectroscopic surveys have uncovered a population of short-period, blended-light spectral binaries composed of low-mass stars and brown dwarfs. These systems are amenable to orbit determination and individual mass measurements via astrometric monitoring. Here, we present first results of a multiyear campaign to obtain high-precision absolute astrometry for spectral binaries using the Gemini-South and Gemini-North GMOS imagers. We measure the complete astrometric orbits for two systems: 2M0805+48 and 2M1059-21. Our astrometric orbit of 2M0805+48 is consistent with its 2-yr radial velocity orbit determined previously and we find a mass of 66<SUB>-14</SUB><SUP>+5</SUP> M<SUB>Jup</SUB> for its T5.5 companion. For 2M1059-21, we find a 1.9-yr orbital period and a mass of 67<SUB>-5</SUB><SUP>+4</SUP> M<SUB>Jup</SUB> for its T3.5 companion. We demonstrate that sub-milliarcsecond absolute astrometry can be obtained with both GMOS imagers and that this is an efficient avenue for confirming and characterizing ultracool binary systems.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enbinaries: close
dc.subject.enbrown dwarfs
dc.subject.enastrometry
dc.subject.enparallaxes
dc.subject.enstars: low-mass
dc.title.enAstrometric orbits of spectral binary brown dwarfs - I. Massive T dwarf companions to 2M1059-21 and 2M0805+48
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/staa1235
dc.subject.halPlanète et Univers [physics]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2004.14889
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page1136-1147
bordeaux.volume495
bordeaux.peerReviewedoui
hal.identifierinsu-03678867
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//insu-03678867v1
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