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: 20 mar. 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 mar. 20 ] -
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 mar. 20 ] - 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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