Fonte: Astronomical Journal. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
ABNT
ROSSI, Silvia Cristina Fernandes et al. Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman. Astronomical Journal, v. 130, p. 2804-2823, 2006Tradução . . Acesso em: 30 set. 2024.APA
Rossi, S. C. F., Beers, T. C., Sneden, C., Sevastyanenko, T., Rhee, J., & Marsteller, B. (2006). Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman. Astronomical Journal, 130, 2804-2823.NLM
Rossi SCF, Beers TC, Sneden C, Sevastyanenko T, Rhee J, Marsteller B. Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman. Astronomical Journal. 2006 ; 130 2804-2823.[citado 2024 set. 30 ]Vancouver
Rossi SCF, Beers TC, Sneden C, Sevastyanenko T, Rhee J, Marsteller B. Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman. Astronomical Journal. 2006 ; 130 2804-2823.[citado 2024 set. 30 ]