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: 04 mar. 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 mar. 04 ] -
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 mar. 04 ] - Broadband UBVRcIc photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I.
- Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5
- The Hamburg/ESO R-process enhanced star survey (HERES): II. Spectroscopic analysis of the survey sample
- Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey
- Estimativas de precisão de temperaturas efetivas estelares e avermelhamento interestelar utilizando o índice de linha de Balmer baseado em espectroscopia de média resolução
- Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields
- The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey
- Elemental abundances and classification of carbon-enhanced metal-poor stars
- Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
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