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dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBarbuy, Beatrizpt_BR
dc.date.accessioned2014-04-15T01:50:50Zpt_BR
dc.date.issued2013pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/94342pt_BR
dc.description.abstractDeep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy.Ayoung age of 3.2 Gyr is found, differently from a previous estimate of 12Gyr. It also appears to be moderately metal rich with [Fe/H]∼−0.8, rather than [Fe/H]∼−1.7, as previously suggested by Fadely et al. A main difference in the age derivation relative to Fadely et al. comes from the consideration of subgiant branch stars in the isochrone fitting. A deduced distance of d = 29.1 kpc is compatible with the outer halo location of other low luminosity globular clusters.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the royal astronomical society. Oxford. Vol. 433, no. 3 (Aug. 2013), p. 1966-1969pt_BR
dc.rightsOpen Accessen
dc.subjectEvolucao estelarpt_BR
dc.subjectHertzsprungen
dc.subjectRussell and colouren
dc.subjectAglomerados estelares globularespt_BR
dc.subjectEstrelas gigantespt_BR
dc.subjectMagnitude diagramsen
dc.subjectHalospt_BR
dc.subjectGlobular clusters: individualen
dc.subjectSegue 3en
dc.subjectGalaxy: haloen
dc.titleSegue 3 : the youngest globular cluster in the outer halopt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000903099pt_BR
dc.type.originEstrangeiropt_BR


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