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dc.contributor.authorBarbuy, Beatrizpt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBonatto, Charles Josept_BR
dc.date.accessioned2014-07-29T02:04:49Zpt_BR
dc.date.issued2006pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98862pt_BR
dc.description.abstractWe present BVI photometry of the globular cluster NGC 6642 using the SOI imager at the SOAR Telescope. The colour magnitude diagrams (CMD) reach ≈ 1.5 mag in V below the main sequence turn-off. A comparison of the overall sequences, and in particular the Red Giant Branch slope of NGC 6642 with that of M 5, indicates that the two clusters must have a similar metallicity of [Fe/H] ≈ –1.3. We also obtained a reddening E(B − V) = 0.42 ± 0.03 for NGC 6642, and a distance from the Sun of dʘ = 7.2 ± 0.5 kpc. Therefore NGC 6642 is a moderately metal-poor globular cluster that is spatially located in the bulge at a galactocentric distance of RGC ≈ 1.7 kpc. The comparison of CMDs of NGC 6642 with those of M 5 shows that there is a very good match of magnitude difference between turn-off and horizontal branch, suggesting comparable ages. The age of M 5 is typical of halo globulars, so NGC 6642 is coeval with the halo. It is a good candidate as one of the few genuine metal-poor and old bulge clusters, and might be one of the oldest fossils in the Galaxy.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. Berlin. Vol. 449, no. 3 (Apr. 2006), p. 1019-1024pt_BR
dc.rightsOpen Accessen
dc.subjectAstronomiapt_BR
dc.subjectGlobular clusters: individual: NGC 6642en
dc.subjectAstrofísicapt_BR
dc.subjectHertzsprung-Russell (HR) and C-M diagramsen
dc.titleSOAR BVI photometry of the metal-poor bulge globular cluster NGC 6642pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000559248pt_BR
dc.type.originEstrangeiropt_BR


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