High quality seeing V, I and Gunn z imaging of Terzan 4 : a blue horizontal branch bulge globular cluster
dc.contributor.author | Ortolani, Sergio | pt_BR |
dc.contributor.author | Barbuy, Beatriz | pt_BR |
dc.contributor.author | Bica, Eduardo Luiz Damiani | pt_BR |
dc.date.accessioned | 2014-07-23T02:04:37Z | pt_BR |
dc.date.issued | 1997 | pt_BR |
dc.identifier.issn | 0004-6361 | pt_BR |
dc.identifier.uri | http://hdl.handle.net/10183/98384 | pt_BR |
dc.description.abstract | We study the globular cluster Terzan 4 projected close to the Galactic center, by means of V, I and Gunn z Colour-Magnitude Diagrams. The images were obtained under exceptional seeing conditions (0.35" - 0.55") at the ESO New Technology Telescope equipped with SUSI. We derive a reddening of E(B-V) = 2.35 amd a distance from the Sun dΘ = 8.3 kpc for Terzan 4. From the similarity of the VI Colour-Magnitude Diagrams of Terzan 4 and M30, in particular the presence of a blue horizontal branch, it could be as metal-poor as [Fe/H] ≈ -2.0. It is therefore another blue horizontal branch globular cluster located close to the Galactic center. | en |
dc.format.mimetype | application/pdf | pt_BR |
dc.language.iso | eng | pt_BR |
dc.relation.ispartof | Astronomy and Astrophysics. Berlin. Vol. 319, no. 3 (Mar. 1997), p. 850-854 | pt_BR |
dc.rights | Open Access | en |
dc.subject | Astrofisica extragalatica | pt_BR |
dc.subject | Globular clusters: individual: Terzan 4;M 30; general | en |
dc.subject | HR diagram | en |
dc.subject | Aglomerados globulares | pt_BR |
dc.subject | Galaxy: center | en |
dc.title | High quality seeing V, I and Gunn z imaging of Terzan 4 : a blue horizontal branch bulge globular cluster | pt_BR |
dc.type | Artigo de periódico | pt_BR |
dc.identifier.nrb | 000157707 | pt_BR |
dc.type.origin | Estrangeiro | pt_BR |
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