Source: The galaxy disk in cosmological context : proceedings. Conference titles: IAU Symposium. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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: 23 maio 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 maio 23 ]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 maio 23 ]