Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields (2006)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: CATÁLOGOS; GALÁXIAS; ABUNDÂNCIAS (ASTRONOMIA); GALÁXIA (VIA LÁCTEA); ABUNDÂNCIA ESTELAR; POPULAÇÕES ESTELARES; ESTRELAS; CARBONO; ESPECTROSCOPIA
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 652, p. 1585-1603, 2006
-
ABNT
FREBEL, Anna et al. Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields. The Astrophysical Journal, v. 652, p. 1585-1603, 2006Tradução . . Disponível em: http://iopscience.iop.org/0004-637X/652/2/1585/pdf/0004-637X_652_2_1585.pdf. Acesso em: 14 fev. 2026. -
APA
Frebel, A., Christlieb, N., Norris, J. E., Beers, T. C., Bessell, M. S., Rhee, J., et al. (2006). Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields. The Astrophysical Journal, 652, 1585-1603. Recuperado de http://iopscience.iop.org/0004-637X/652/2/1585/pdf/0004-637X_652_2_1585.pdf -
NLM
Frebel A, Christlieb N, Norris JE, Beers TC, Bessell MS, Rhee J, Fechner C, Marsteller B, Rossi SCF, Thom C, Wisotzki L, Reimers D. Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields [Internet]. The Astrophysical Journal. 2006 ; 652 1585-1603.[citado 2026 fev. 14 ] Available from: http://iopscience.iop.org/0004-637X/652/2/1585/pdf/0004-637X_652_2_1585.pdf -
Vancouver
Frebel A, Christlieb N, Norris JE, Beers TC, Bessell MS, Rhee J, Fechner C, Marsteller B, Rossi SCF, Thom C, Wisotzki L, Reimers D. Bright metal-poor stars from the Hamburg/ESO survey: I. Selection and follow-up observations from 329 fields [Internet]. The Astrophysical Journal. 2006 ; 652 1585-1603.[citado 2026 fev. 14 ] Available from: http://iopscience.iop.org/0004-637X/652/2/1585/pdf/0004-637X_652_2_1585.pdf - 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
- 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
- High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725
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