Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey (1999)
- Authors:
- Autor USP: ROSSI, SILVIA CRISTINA FERNANDES - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Publisher: Astronomical Society of the Pacific
- Publisher place: Australia
- Date published: 1999
- Source:
- Título: Proceedings
- Conference titles: Stromlo Symposium the Galactic Halo
-
ABNT
BEERS, Timothy C. e ROSSI, Silvia Cristina Fernandes. Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey. 1999, Anais.. Australia: Astronomical Society of the Pacific, 1999. . Acesso em: 13 fev. 2026. -
APA
Beers, T. C., & Rossi, S. C. F. (1999). Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey. In Proceedings. Australia: Astronomical Society of the Pacific. -
NLM
Beers TC, Rossi SCF. Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey. Proceedings. 1999 ;[citado 2026 fev. 13 ] -
Vancouver
Beers TC, Rossi SCF. Metal abundance estimates for F- and G-type stars from Edinburgh-cape blue object survey. Proceedings. 1999 ;[citado 2026 fev. 13 ] - 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
- 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
- High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725
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