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dc.contributor.authorCampos, Fabíolapt_BR
dc.contributor.authorPelisoli, Ingrid Domingospt_BR
dc.contributor.authorKamann, Sebastianpt_BR
dc.contributor.authorHusser, Tim Oliverpt_BR
dc.contributor.authorDreizler, Stefanpt_BR
dc.contributor.authorBellini, Andreapt_BR
dc.contributor.authorRobinson, E.L.pt_BR
dc.contributor.authorNardiello, Domenicopt_BR
dc.contributor.authorPiotto, Giampaolopt_BR
dc.contributor.authorKepler, Souza Oliveirapt_BR
dc.contributor.authorIstrate, Alina G.pt_BR
dc.contributor.authorWinget, Donald Earlpt_BR
dc.contributor.authorMontgomery, Michael Houstonpt_BR
dc.contributor.authorDotter, Aaron Loverenpt_BR
dc.date.accessioned2019-06-13T02:31:21Zpt_BR
dc.date.issued2018pt_BR
dc.identifier.issn0035-8711pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/195761pt_BR
dc.description.abstractWe use Hubble Space Telescope multicolour photometry of the globular cluster 47 Tucanae to uncover a population of 24 objects with no previous classification that are outliers from the single-star model tracks in the colour–magnitude diagram and yet are likely cluster members. By comparing those sources with evolutionary models and X-ray source catalogues, we were able to show that the majority of those sources are likely binary systems that do not have any X-ray source detected nearby, most possibly formed by a white dwarf and a main-sequence star and a small number of possible double-degenerate systems.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofMonthly notices of the royal astronomical society. Oxford. Vol. 481, no. 4 (Dec. 2018), p. 4397–4409pt_BR
dc.rightsOpen Accessen
dc.subjectAnãs brancaspt_BR
dc.subjectAglomerados globularespt_BR
dc.subjectFotometria astronômicapt_BR
dc.titleOutliers : multicolour photometry guiding the search for evolved binary systems in the globular cluster 47Tucanaept_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001090626pt_BR
dc.type.originEstrangeiropt_BR


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