New grids of synthetic spectra for abundance derivation and population synthesis (1999)
- Authors:
- USP affiliated author: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- School: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Astronomical Society Pacific
- Place of publication: San Francisco
- Date published: 1999
- Source:
- Título do periódico: The stellar content of local group galaxies : proceedings
- Conference title: International Astronomical Union Symposium
-
ABNT
BARBUY, Beatriz Leonor Silveira; PERRIN, M. N.; CAYREL, R.; et al. New grids of synthetic spectra for abundance derivation and population synthesis. Anais.. San Francisco: Astronomical Society Pacific, 1999. -
APA
Barbuy, B. L. S., Perrin, M. N., Cayrel, R., Katz, D., Veer, C. V. 't, & Schiavon, R. P. (1999). New grids of synthetic spectra for abundance derivation and population synthesis. In The stellar content of local group galaxies : proceedings. San Francisco: Astronomical Society Pacific. -
NLM
Barbuy BLS, Perrin MN, Cayrel R, Katz D, Veer CV't, Schiavon RP. New grids of synthetic spectra for abundance derivation and population synthesis. The stellar content of local group galaxies : proceedings. 1999 ; -
Vancouver
Barbuy BLS, Perrin MN, Cayrel R, Katz D, Veer CV't, Schiavon RP. New grids of synthetic spectra for abundance derivation and population synthesis. The stellar content of local group galaxies : proceedings. 1999 ; - VLT-UVES Spectroscopy of the subgiant I-24 of the bulge globular cluster NGC 6528 in baade´s window
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- 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
- The distance and space distribution of bulge globular clusters
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