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dc.contributor.authorBarbuy, Beatrizpt_BR
dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorDesidera, S.pt_BR
dc.date.accessioned2014-07-18T02:04:26Zpt_BR
dc.date.issued1999pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98060pt_BR
dc.description.abstractWe present V and I photometry for the bulge globular cluster NGC 6401 for the first time. The Colour-Magnitude Diagram reveals a red horizontal branch, and the cluster is metalrich ([Fe/H] ≈ -0.7). NGC 6401 is located at 5.3° from the Galactic center, turning out to be an interesting target to trace the extent of the bulge. A reddening E(B-V) = 0.53 ± 0.15 and a distance from the Sun dʘ ≈ 12.0 ± 1.0 kpc are derived. The cluster is slightly behind the bulk of the bulge population in that direction, but still within the bulge volume. Since the number of clusters with Horizontal Branch information has increased enormously in the later years for the central 20° x 20° , we present a discussion on the distribution of red and blue horizontal branch clusters and their possible relation to bulge and/or halo.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and astrophysics. Berlin. Vol. 348, no. 3 (Aug. 1999), p. 783-788pt_BR
dc.rightsOpen Accessen
dc.subjectStars: Hertzsprungen
dc.subjectAglomerados estelares globularespt_BR
dc.subjectEvolucao estelarpt_BR
dc.subjectRussel (HR) and C-M diagramsen
dc.subjectFotometriapt_BR
dc.subjectGalaxy: globular clusters: individual: NGC6401en
dc.titleThe metal-rich bulge globular cluster NGC 6401pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000270027pt_BR
dc.type.originEstrangeiropt_BR


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