Chemical abundances in metal-rich bulge-like stars (2007)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Subjects: ABUNDÂNCIA ESTELAR; FORMAÇÃO E EVOLUÇÃO DA GALÁXIA; ESTRELAS
- Language: Inglês
- Imprenta:
- Publisher: Cambridge Unversity Press
- Publisher place: Cambridge
- Date published: 2007
- Source:
- Conference titles: Symposium of the International Astronomical Union
-
ABNT
POMPEIA, L et al. Chemical abundances in metal-rich bulge-like stars. 2007, Anais.. Cambridge: Cambridge Unversity Press, 2007. . Acesso em: 04 ago. 2025. -
APA
Pompeia, L., Barbuy, B. L. S., Grenon, M., & Gustafsson, B. (2007). Chemical abundances in metal-rich bulge-like stars. In Stellar populations of building blocks of galaxies: Proceedings. Cambridge: Cambridge Unversity Press. -
NLM
Pompeia L, Barbuy BLS, Grenon M, Gustafsson B. Chemical abundances in metal-rich bulge-like stars. Stellar populations of building blocks of galaxies: Proceedings. 2007 ;[citado 2025 ago. 04 ] -
Vancouver
Pompeia L, Barbuy BLS, Grenon M, Gustafsson B. Chemical abundances in metal-rich bulge-like stars. Stellar populations of building blocks of galaxies: Proceedings. 2007 ;[citado 2025 ago. 04 ] - A fossil bulge globular cluster revealed by very large telescope multi-conjugate adaptative optics
- First stars: XIII. Two extremely metal-poor RR Lyrae stars
- First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity
- First stars VI-abundances of 'C', 'N', 'O', 'Li', and mixing in extremely metal-poor giants. galactic evolution of the light elements
- r-Process abundances in metal-poor Galactic halo stars
- Pfleiderer 2: identification of a new globular cluster in the galaxy
- B,V and V,I color-magnitude diagrams of 'omega' centauri compared to templates
- New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: binarity and neutron capture elements
- NGC 6553: a detailed abundance analysis as a tracer of the chemical evolution in the galaxy
- Chemical abundances in the galactic bulge: evidence for a fast enrichment
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