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dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBarbuy, Beatrizpt_BR
dc.date.accessioned2014-07-18T02:04:34Zpt_BR
dc.date.issued1995pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98076pt_BR
dc.description.abstractWe present NTT V,I observations of Palomar 6 and Djorgovski 1, two obscured loose clusters in crowded fields. We derive a reddening of E(B - V) = 1.33 ± 0.10, a distance dʘ ≈ 8.9 kpc, and a metallicity of [Fe/H] ≈ -0.4 for Pal 6, and E(B- V)= 1.71 ± 0.10, dʘ ≈ 8.8kpc, and a similar metallicity ([Fe/H] ≈ -0.4) for Djorg 1.en
dc.format.mimetypeapplication/pdf
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. Berlin. Vol. 296, no. 3 (Apr. 1995), p. 680-684pt_BR
dc.rightsOpen Accessen
dc.subjectGlobular clusters: generalen
dc.subjectAstronomia extragalaticapt_BR
dc.subjectPal 6en
dc.subjectAglomerados globularespt_BR
dc.subjectEvolucao estelarpt_BR
dc.subjectDjorg 1 - HR diagrammen
dc.titleTwo reddened globular cluster projected close to the galactic center : Palomar 6 and Djorgovski 1pt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000262714pt_BR
dc.type.originEstrangeiropt_BR


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