Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman (2006)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v. 130, p. 2804-2823, 2006
-
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: 09 jan. 2026. -
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 2026 jan. 09 ] -
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 2026 jan. 09 ] - A catalog of candidate field horizontal-branch and a-type stars: III. A 2 mass-cheaned version
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