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dc.contributor.authorFaifer, Favio Raúlpt_BR
dc.contributor.authorEscudero, Carlos G.pt_BR
dc.contributor.authorCastelli, Analía Smithpt_BR
dc.contributor.authorForte, Juan Carlospt_BR
dc.contributor.authorSesto, Leandro A.pt_BR
dc.contributor.authorChies-Santos, Ana Leonorpt_BR
dc.contributor.authorCortesi, Ariannapt_BR
dc.contributor.authorOliveira, Claudia Lucia Mendes dept_BR
dc.date.accessioned2018-02-28T02:26:57Zpt_BR
dc.date.issued2017pt_BR
dc.identifier.issn2075-4434pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/172987pt_BR
dc.description.abstractIn this letter, we present preliminary results of the analysis of Flamingos-2 and GMOS-S photometry of the globular cluster (GC) system of the elliptical galaxy NGC1395. This is the first step of a long-term Brazilian–Argentinian collaboration for the study of GC systems in early-type galaxies. In the context of this collaboration, we obtained deep NIR photometric data in two different bands (J and Ks), which were later combined with high quality optical Gemini + GMOS photometry previously obtained by the Argentinian team. This allowed us to obtain different color indices, less sensitive to the effect of horizontal branch (HB) stars for several hundreds of GC candidates, and to make an initial assessment of the presence or absence of multiple GC populations in colors in NGC1395.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofGalaxies. Basel. Vol. 5, no. 3 (Sept. 2017), 38, 6 p.pt_BR
dc.rightsOpen Accessen
dc.subjectEarly-type galaxiesen
dc.subjectAglomerados globularespt_BR
dc.subjectGaláxia NGC 1395pt_BR
dc.subjectGlobular clusteren
dc.subjectGalaxy halosen
dc.subjectFotometria astronômicapt_BR
dc.titleThe Brazil–Argentina Gemini Group for the study of Globular Cluster Systems (BAGGs GCs) : FLAMINGOS-2 and GMOS data for NGC 1395pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001055933pt_BR
dc.type.originEstrangeiropt_BR


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