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dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorMomany, Yazanpt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBarbuy, Beatrizpt_BR
dc.date.accessioned2014-07-24T02:04:21Zpt_BR
dc.date.issued2000pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98506pt_BR
dc.description.abstractWe presentBandVphotometry of the bulge globular cluster NGC 6304. We derive a reddening E(B-V) 0.5 and a distance from the Sun d 6 kpc. From the red giant branch morphology we estimate that the metallicity of NGC 6304 is intermediate between those of 47 Tuc and NGC 6528. The cluster is foreground to the bulk of the bulge population and the reddenings are comparable. Evidence of a hot stellar component belonging to the cluster is found. These hot stars could correspond to a blue extended horizontal branch and/or blue stragglers.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and astrophysics. New York. Vol. 357, no. 2 (May 2000), p. 495-500pt_BR
dc.rightsOpen Accessen
dc.subjectAglomerados estelarespt_BR
dc.subjectStars: Hertzsprung–Russel (HR) and C-M diagramsen
dc.subjectEvolucao estelarpt_BR
dc.subjectGalaxy: globular clusters: individual: NGC 6304en
dc.subjectFotometria estelarpt_BR
dc.titleB and V photometry of the metal-rich bulge globular cluster NGC 6304pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000274956pt_BR
dc.type.originEstrangeiropt_BR


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