Near-infrared spectroscopy of carbon-enhanced metal-poor stars: I. A SOAR/OSIRIS pilot study (2007)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ABUNDÂNCIA ESTELAR; POPULAÇÕES ESTELARES
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v.133, n.3 p.1193-1203, 2007
-
ABNT
BEERS, Timothy C et al. Near-infrared spectroscopy of carbon-enhanced metal-poor stars: I. A SOAR/OSIRIS pilot study. The Astronomical Journal, v. 133, n. 3 p.1193-1203, 2007Tradução . . Acesso em: 04 mar. 2026. -
APA
Beers, T. C., Rossi, S. C. F., Thirupathi Sivarani, B. M., Lee, Y. S., & Plez, B. (2007). Near-infrared spectroscopy of carbon-enhanced metal-poor stars: I. A SOAR/OSIRIS pilot study. The Astronomical Journal, 133( 3 p.1193-1203). -
NLM
Beers TC, Rossi SCF, Thirupathi Sivarani BM, Lee YS, Plez B. Near-infrared spectroscopy of carbon-enhanced metal-poor stars: I. A SOAR/OSIRIS pilot study. The Astronomical Journal. 2007 ;133( 3 p.1193-1203):[citado 2026 mar. 04 ] -
Vancouver
Beers TC, Rossi SCF, Thirupathi Sivarani BM, Lee YS, Plez B. Near-infrared spectroscopy of carbon-enhanced metal-poor stars: I. A SOAR/OSIRIS pilot study. The Astronomical Journal. 2007 ;133( 3 p.1193-1203):[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
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
