[O/Fe] estimates for carbon-enhanced metal-poor stars from near-infrared spectroscopy (2011)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; ABUNDÂNCIA ESTELAR; POPULAÇÕES ESTELARES; ESPECTROSCOPIA
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v. 141, p. 102/1-102/10, 2011
-
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: 27 jan. 2026. -
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 2026 jan. 27 ] -
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 2026 jan. 27 ] - Additional emission-line candidates from the hk survey
- Spectroscopic validation of low-metallicity stars from RAVE
- High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725
- Identification and analysis of horizontal-branch and other A-type stars in the galaxy
- The age structure of the Milky Way’s halo
- Descoberta e análise de objetos com linhas em emissão no survey HK
- Searching for chemical classes among metal-poor stars using medium-resolution spectroscopy
- Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis
- Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS
- A stellar relic from the early Milky Way
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas