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dc.contributor.authorOrtolani, Sergiopt_BR
dc.contributor.authorBica, Eduardo Luiz Damianipt_BR
dc.contributor.authorBarbuy, Beatrizpt_BR
dc.date.accessioned2014-07-24T02:04:22Zpt_BR
dc.date.issued2000pt_BR
dc.identifier.issn0004-6361pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/98510pt_BR
dc.description.abstractBy means of VI CCD photometry we identify a new globular cluster in the Galaxy: ESO 280−SC06. The images and Colour Magnitude Diagrams indicate that we are dealing with a sparsely populated globular cluster, showing a compact core. The cluster is located in Ara, projected at only 12.6° from the plane, and appears to be metal poor ([Fe/H] ≈ −1:8). We derive a reddening E(B−V) = 0.07 and a distance from the Sun dʘ = 21.9 kpc. It is a halo globular cluster on the opposite side of the Galaxy.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofAstronomy and Astrophysics. New York. Vol. 361, n. 3 (Sept. 2000), p. L57-L59pt_BR
dc.rightsOpen Accessen
dc.subjectAglomerados estelares globularespt_BR
dc.subjectStars: Hertzsprungen
dc.subjectRussel (HR) and C-M diagramsen
dc.subjectFotometria estelarpt_BR
dc.subjectGalaxy: globular clusters: individual: ESO 280–SC06en
dc.titleESO 280-SC06 : a new globular cluster in the galaxypt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb000279538pt_BR
dc.type.originEstrangeiropt_BR


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