Segue 3 : the youngest globular cluster in the outer halo
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 | 2014-04-15T01:50:50Z | pt_BR |
dc.date.issued | 2013 | pt_BR |
dc.identifier.issn | 0035-8711 | pt_BR |
dc.identifier.uri | http://hdl.handle.net/10183/94342 | pt_BR |
dc.description.abstract | Deep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy.Ayoung age of 3.2 Gyr is found, differently from a previous estimate of 12Gyr. It also appears to be moderately metal rich with [Fe/H]∼−0.8, rather than [Fe/H]∼−1.7, as previously suggested by Fadely et al. A main difference in the age derivation relative to Fadely et al. comes from the consideration of subgiant branch stars in the isochrone fitting. A deduced distance of d = 29.1 kpc is compatible with the outer halo location of other low luminosity globular clusters. | en |
dc.format.mimetype | application/pdf | pt_BR |
dc.language.iso | eng | pt_BR |
dc.relation.ispartof | Monthly notices of the royal astronomical society. Oxford. Vol. 433, no. 3 (Aug. 2013), p. 1966-1969 | pt_BR |
dc.rights | Open Access | en |
dc.subject | Evolucao estelar | pt_BR |
dc.subject | Hertzsprung | en |
dc.subject | Russell and colour | en |
dc.subject | Aglomerados estelares globulares | pt_BR |
dc.subject | Estrelas gigantes | pt_BR |
dc.subject | Magnitude diagrams | en |
dc.subject | Halos | pt_BR |
dc.subject | Globular clusters: individual | en |
dc.subject | Segue 3 | en |
dc.subject | Galaxy: halo | en |
dc.title | Segue 3 : the youngest globular cluster in the outer halo | pt_BR |
dc.type | Artigo de periódico | pt_BR |
dc.identifier.nrb | 000903099 | pt_BR |
dc.type.origin | Estrangeiro | pt_BR |
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