Searching for s-process-enhanced metal-poor stars (2009)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ESTRELAS; ABUNDÂNCIAS (ASTRONOMIA); ESPECTROSCOPIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Publications of the Astronomical Society of Australia
- ISSN: 1323-3580
- Volume/Número/Paginação/Ano: v. 26, p. 335-338, 2009
-
ABNT
CRUZ, M.A e ROSSI, Sílvia Cristina Fernandes e BEERS, T.C. Searching for s-process-enhanced metal-poor stars. Publications of the Astronomical Society of Australia, v. 26, p. 335-338, 2009Tradução . . Acesso em: 04 mar. 2026. -
APA
Cruz, M. A., Rossi, S. C. F., & Beers, T. C. (2009). Searching for s-process-enhanced metal-poor stars. Publications of the Astronomical Society of Australia, 26, 335-338. -
NLM
Cruz MA, Rossi SCF, Beers TC. Searching for s-process-enhanced metal-poor stars. Publications of the Astronomical Society of Australia. 2009 ; 26 335-338.[citado 2026 mar. 04 ] -
Vancouver
Cruz MA, Rossi SCF, Beers TC. Searching for s-process-enhanced metal-poor stars. Publications of the Astronomical Society of Australia. 2009 ; 26 335-338.[citado 2026 mar. 04 ] - 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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