[O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy (2011)
Source: The Astronomical Journal. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESPECTROSCOPIA
ABNT
KENNEDY, Catherine R et al. [O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy. The Astronomical Journal, v. 141, p. 102/1-102/10, 2011Tradução . . Acesso em: 17 out. 2024.APA
Kennedy, C. R., Sivarani, T., Beers, T. C., Young, S. L., Placco, V. M., Rossi, S. C. F., et al. (2011). [O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy. The Astronomical Journal, 141, 102/1-102/10.NLM
Kennedy CR, Sivarani T, Beers TC, Young SL, Placco VM, Rossi SCF, Christlieb N, Herwig F, Plez B. [O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy. The Astronomical Journal. 2011 ; 141 102/1-102/10.[citado 2024 out. 17 ]Vancouver
Kennedy CR, Sivarani T, Beers TC, Young SL, Placco VM, Rossi SCF, Christlieb N, Herwig F, Plez B. [O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy. The Astronomical Journal. 2011 ; 141 102/1-102/10.[citado 2024 out. 17 ]