Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg

Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg (2009)

Authors:
Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR; ATMOSFERAS ESTELARES; POPULAÇÕES ESTELARES; FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
Language: Inglês
Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2009
Source:
- Título do periódico: The galaxy disk in cosmological context : proceedings
Conference titles: IAU Symposium

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ABNT

SPITE, M et al. Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg. 2009, Anais.. Paris: International Astronomical Union, 2009. . Acesso em: 24 abr. 2024.
APA

Spite, M., Bonifácio, P., Cayrel, R., & Barbuy, B. L. S. (2009). Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg. In The galaxy disk in cosmological context : proceedings. Paris: International Astronomical Union.
NLM

Spite M, Bonifácio P, Cayrel R, Barbuy BLS. Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg. The galaxy disk in cosmological context : proceedings. 2009 ;[citado 2024 abr. 24 ]
Vancouver

Spite M, Bonifácio P, Cayrel R, Barbuy BLS. Halo chemistry and first stars. The chemical composition of the matter in the early Galaxy, from C to Mg. The galaxy disk in cosmological context : proceedings. 2009 ;[citado 2024 abr. 24 ]