The distance and space distribution of bulge globular clusters (2010)
- Authors:
- USP affiliated author: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- School: IAG
- Subjects: ESTRUTURA DA GALÁXIA; AGLOMERADOS (GALÁXIA)
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University Press
- Place of publication: Cambridge
- Date published: 2010
- Source:
- Título do periódico: Stars clusters : basic galactic building throughout time and space. Proceedings
- ISSN: 1743-9213
- Conference title: IAU Symposium
-
ABNT
ORTOLANI, Sérgio e BARBUY, Beatriz Leonor Silveira e BICA, Eduardo. The distance and space distribution of bulge globular clusters. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 02 jul. 2022. -
APA
Ortolani, S., Barbuy, B. L. S., & Bica, E. (2010). The distance and space distribution of bulge globular clusters. In Stars clusters : basic galactic building throughout time and space. Proceedings. Cambridge: Cambridge University Press. -
NLM
Ortolani S, Barbuy BLS, Bica E. The distance and space distribution of bulge globular clusters. Stars clusters : basic galactic building throughout time and space. Proceedings. 2010 ;[citado 2022 jul. 02 ] -
Vancouver
Ortolani S, Barbuy BLS, Bica E. The distance and space distribution of bulge globular clusters. Stars clusters : basic galactic building throughout time and space. Proceedings. 2010 ;[citado 2022 jul. 02 ] - VLT-UVES Spectroscopy of the subgiant I-24 of the bulge globular cluster NGC 6528 in baade´s window
- Mapping out the interstellar extinction in the central 10 degrees of the galaxy with 2MASS
- New infrared star clusters in the Northern and Equatorial milky way with 2MASS
- First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,*
- Lead abundance in the uranium star CS 31082-001
- Aglomerados globulares das nuvens de Magalhães: idade e metalicidades
- A new approach to derive ['alfa'/Fe] for integrated stellar populations
- Metal-poor globular clusters of the galactic bulge
- Physical parameters of intermediate-age LMC clusters from modelling of HST CMDs
- Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg
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