Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS (2010)
- Autores:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Assuntos: ABUNDÂNCIA ESTELAR; GALÁXIAS; CARBONO
- Idioma: Inglês
- Imprenta:
- Editora: Cambridge University Press
- Local: Cambridge
- Data de publicação: 2010
- Fonte:
- Título do periódico: Chemical abundances in the Universe : connecting first stars to planets. Proceedings
- ISSN: 1743-9213
- Nome do evento: IAU Symposium
-
ABNT
KENNEDY, Catherine R et al. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 20 abr. 2024. -
APA
Kennedy, C. R., Sivarani, T., Beers Thimothy C,, Rossi, S. C. F., Placco, V. M., Johnson, J., & Masseron, T. (2010). Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. In Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Cambridge: Cambridge University Press. -
NLM
Kennedy CR, Sivarani T, Beers Thimothy C, Rossi SCF, Placco VM, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 abr. 20 ] -
Vancouver
Kennedy CR, Sivarani T, Beers Thimothy C, Rossi SCF, Placco VM, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 abr. 20 ] - Descoberta e análise de objetos com linhas em emissão no Survey HK
- A search for unrecognized carbon-enchanced metal-poor stars
- s/r ratios in carbon-enhanced metal-poor stars
- Stellar spectra
- A continued search for CEMP RR Lyrae stars
- Searching for s-process-enhanced metal-poor stars
- Estimation of carbon abundances in metal-poor stars. I. application to the strong g-band stars of beers, preston, and shectman
- The stellar content of the Hamburg/ESO survey: III. field horizontal-branch stars in the galaxy
- The ideal stars for exploration of early-epoch 'ANTIPOT.7 LI' abundances
- Spectroscopic validation of low-metallicity stars from RAVE
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