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dc.contributor.authorTEIXEIRA, R.,
hal.structure.identifierM2A 2014
dc.contributor.authorDUCOURANT, C.
dc.contributor.authorKRONE-MARTINS, A.,
dc.contributor.authorSCARANO, S.,
hal.structure.identifierSIM/IDL Faculdade de Ciências da Universidade de Lisboa [FCUL]
dc.contributor.authorMOITINHO, A.,
dc.contributor.authorGALLI, Ph.,
dc.date.issued2014
dc.identifier.issn0037-8720
dc.description.abstractEnBrown dwarfs are extremely important objects for our understanding of stellar and planetary formation and evolution. Lying at the limit of the coolest stars, they are poorly understood and the atmospheric models of are not yet reliable. Beyond this population, very cool brown dwarfs (Teff˜300 K) were recently discovered constituting new spectral classes. A precise distance is the fundamental parameter to be able to correctly derive their masses, ages and thus calibrate the atmospheric models of this type of object. In 2012 we started an observational program to measure the trigonometric parallax of 5 such extreme objects recently detected prototypes of cool brown dwarfs. Observations started at the 4.1m SOAR/Spartan telescope and will continue until the end of 2014. Here we present an overview on the development of this project.
dc.language.isoen
dc.publisherSocietà astronomica italiana
dc.subject.enStars: brown dwarf
dc.subject.enStars: trigonometric parallax
dc.subject.enStars: formation
dc.title.enParallaxes of ultra cool brown dwarf calibrators.
dc.typeArticle de revue
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.journalMemorie della Societa astronomica italiana
bordeaux.page793
bordeaux.volume85
bordeaux.peerReviewedoui
hal.identifierhal-01153848
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01153848v1
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