The frequency of carbon-enhanced metal-poor stars in the galaxy from the heres sample (2006)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTROFÍSICA; GALÁXIAS; MEIO INTERGALÁTICO
- Language: Inglês
- Imprenta:
- Source:
- Título: Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 652, p. L37-L40, 2006
-
ABNT
LUCATELLO, Sara et al. The frequency of carbon-enhanced metal-poor stars in the galaxy from the heres sample. Astrophysical Journal, v. 652, p. L37-L40, 2006Tradução . . Acesso em: 10 mar. 2026. -
APA
Lucatello, S., Beers, T. C., Christlieb, N., Barklem, P. S., Rossi, S. C. F., Marsteller, B., et al. (2006). The frequency of carbon-enhanced metal-poor stars in the galaxy from the heres sample. Astrophysical Journal, 652, L37-L40. -
NLM
Lucatello S, Beers TC, Christlieb N, Barklem PS, Rossi SCF, Marsteller B, Sivarani T, Lee YS. The frequency of carbon-enhanced metal-poor stars in the galaxy from the heres sample. Astrophysical Journal. 2006 ; 652 L37-L40.[citado 2026 mar. 10 ] -
Vancouver
Lucatello S, Beers TC, Christlieb N, Barklem PS, Rossi SCF, Marsteller B, Sivarani T, Lee YS. The frequency of carbon-enhanced metal-poor stars in the galaxy from the heres sample. Astrophysical Journal. 2006 ; 652 L37-L40.[citado 2026 mar. 10 ] - 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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