New grids of synthetic spectra for abundance derivation and population synthesis (1999)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Astronomical Society Pacific
- Publisher place: San Francisco
- Date published: 1999
- Source:
- Título do periódico: The stellar content of local group galaxies : proceedings
- Conference titles: International Astronomical Union Symposium
-
ABNT
BARBUY, Beatriz Leonor Silveira et al. New grids of synthetic spectra for abundance derivation and population synthesis. 1999, Anais.. San Francisco: Astronomical Society Pacific, 1999. . Acesso em: 07 maio 2024. -
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 ;[citado 2024 maio 07 ] -
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 ;[citado 2024 maio 07 ] - O processo s e as estrelas de bário
- Alpha & heavy elements abundances of nearby bulgelike dwarf stars
- Who´s who among barium stars
- The galactic bulge
- Efeitos do mixing nas abundâncias de CNO em supergigantes frias
- Chemical composition and stellar populations of the galactic bulge
- Abundances in extremely metal-poor stars: comparison of the trends of abundance ratios in giants and turn off stars
- Oxigênio em aglomerados pobres em metais do bojo: HP1 e NGC6558
- Oxigênio em aglomerados pobres em metais do bojo: HP1 e NGC 6558
- Abundances in the Galactic Bulge: evidence for fast chemical enrichment
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