ESO 280-SC06 : a new globular cluster in the galaxy
dc.contributor.author | Ortolani, Sergio | pt_BR |
dc.contributor.author | Bica, Eduardo Luiz Damiani | pt_BR |
dc.contributor.author | Barbuy, Beatriz | pt_BR |
dc.date.accessioned | 2014-07-24T02:04:22Z | pt_BR |
dc.date.issued | 2000 | pt_BR |
dc.identifier.issn | 0004-6361 | pt_BR |
dc.identifier.uri | http://hdl.handle.net/10183/98510 | pt_BR |
dc.description.abstract | By 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.mimetype | application/pdf | pt_BR |
dc.language.iso | eng | pt_BR |
dc.relation.ispartof | Astronomy and Astrophysics. New York. Vol. 361, n. 3 (Sept. 2000), p. L57-L59 | pt_BR |
dc.rights | Open Access | en |
dc.subject | Aglomerados estelares globulares | pt_BR |
dc.subject | Stars: Hertzsprung | en |
dc.subject | Russel (HR) and C-M diagrams | en |
dc.subject | Fotometria estelar | pt_BR |
dc.subject | Galaxy: globular clusters: individual: ESO 280–SC06 | en |
dc.title | ESO 280-SC06 : a new globular cluster in the galaxy | pt_BR |
dc.type | Artigo de periódico | pt_BR |
dc.identifier.nrb | 000279538 | pt_BR |
dc.type.origin | Estrangeiro | pt_BR |
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