A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy (2013)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ESTRELAS; GALÁXIA (VIA LÁCTEA); CARBONO
- Language: Inglês
- Imprenta:
- Publisher: American Astronomical Society
- Publisher place: Washington
- Date published: 2013
- Conference titles: AAS Meeting
-
ABNT
BEERS, T. C et al. A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy. 2013, Anais.. Washington: American Astronomical Society, 2013. . Acesso em: 28 jan. 2026. -
APA
Beers, T. C., Placco, V., Rossi, S. C. F., Christlieb, N., & Kennedy, C. (2013). A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy. In . Washington: American Astronomical Society. -
NLM
Beers TC, Placco V, Rossi SCF, Christlieb N, Kennedy C. A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy. 2013 ;[citado 2026 jan. 28 ] -
Vancouver
Beers TC, Placco V, Rossi SCF, Christlieb N, Kennedy C. A new survey for carbon-enhanced metal-poor stars in the halo(es) of the Galaxy. 2013 ;[citado 2026 jan. 28 ] - 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
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