Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS (2009)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: GALÁXIA (VIA LÁCTEA); CENTRO GALÁCTICO
- Language: Inglês
- Imprenta:
- Publisher: American Astronomical Society
- Publisher place: Washington
- Date published: 2009
- Conference titles: Meeting of the American Astronomical Society with HAD and HEAD
-
ABNT
KENNEDY, Catherine R et al. Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS. 2009, Anais.. Washington: American Astronomical Society, 2009. . Acesso em: 27 jan. 2026. -
APA
Kennedy, C. R., Sivarani, T., Beers, T., Rossi, S. C. F., Placco, V., Johnson, J., & Masseron, T. (2009). Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS. In . Washington: American Astronomical Society. -
NLM
Kennedy CR, Sivarani T, Beers T, Rossi SCF, Placco V, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS. 2009 ;[citado 2026 jan. 27 ] -
Vancouver
Kennedy CR, Sivarani T, Beers T, Rossi SCF, Placco V, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/ OSIRIS. 2009 ;[citado 2026 jan. 27 ] - Additional emission-line candidates from the hk survey
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- 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
- A stellar relic from the early Milky Way
- A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy
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