Journal article
The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge
Monthly notices of the Royal Astronomical Society, Vol.445(4), pp.4241-4246
12/21/2014
DOI: 10.1093/mnras/stu1991
Abstract
We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars should now preferentially reside. EMBLA utilizes SkyMapper photometry to pre-select metal-poor candidates, which are subsequently confirmed using AAOmega spectroscopy. We describe the discovery and analysis of four bulge giants with -2.72 <= [Fe/H] <= -2.48, the lowest metallicity bulge stars studied with high-resolution spectroscopy to date. Using FLAMES/UVES spectra through the Gaia-ESO Survey we have derived abundances of twelve elements. Given the uncertainties, we find a chemical similarity between these bulge stars and halo stars of the same metallicity, although the abundance scatter may be larger, with some of the stars showing unusual [alpha/Fe] ratios.
Details
- Title: Subtitle
- The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge
- Creators
- L. M. Howes - Australian National UniversityM. Asplund - Australian National UniversityA. R. Casey - University of CambridgeS. C. Keller - Australian National UniversityD. Yong - Australian National UniversityG. Gilmore - University of CambridgeK. Lind - Uppsala UniversityC. Worley - University of CambridgeM. S. Bessell - Australian National UniversityL. Casagrande - Australian National UniversityA. F. Marino - Australian National UniversityD. M. Nataf - Australian National UniversityC. I. Owen - Australian National UniversityG. S. Da Costa - Australian National UniversityB. P. Schmidt - Australian National UniversityP. Tisserand - Australian National UniversityS. Randich - Arcetri Astrophysical ObservatoryS. Feltzing - Lund UniversityA. Vallenari - Osservatorio Astronomico di PadovaC. Allende Prieto - Inst Astrofis Canarias, E-38205 Tenerife, SpainT. Bensby - Lund UniversityE. Flaccomio - Osservatorio Astronomico di PalermoA. J. Korn - Uppsala UniversityE. Pancino - Osservatorio astronomico di BolognaA. Recio-Blanco - Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, Lab Lagrange,UMR7293, F-06304 Nice 4, FranceR. Smiljanic - Nicolaus Copernicus Astronomical CenterM. Bergemann - University of CambridgeM. T. Costado - Instituto de Astrofísica de AndalucíaF. Damiani - Osservatorio Astronomico di PalermoU. Heiter - Uppsala UniversityV. Hill - Observatoire de la Côte d’AzurA. Hourihane - University of CambridgeP. Jofre - University of CambridgeC. Lardo - Osservatorio astronomico di BolognaP. de laverny - Observatoire de la Côte d’AzurL. Magrini - Arcetri Astrophysical ObservatoryE. Maiorca - Arcetri Astrophysical ObservatoryT. Masseron - University of CambridgeL. Morbidelli - Arcetri Astrophysical ObservatoryG. G. Sacco - Arcetri Astrophysical ObservatoryD. Minniti - Millennium Institute of AstrophysicsM. Zoccali - Millennium Institute of Astrophysics
- Resource Type
- Journal article
- Publication Details
- Monthly notices of the Royal Astronomical Society, Vol.445(4), pp.4241-4246
- Publisher
- Oxford Univ Press
- DOI
- 10.1093/mnras/stu1991
- ISSN
- 0035-8711
- eISSN
- 1365-2966
- Number of pages
- 6
- Grant note
- FL110100012; DP120101237 / Australian Research Council 1110393 / Fondecyt; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT); CONICYT FONDECYT RPG-2012-541 / Leverhulme Trust INAF; Istituto Nazionale Astrofisica (INAF) PFB-06 / BASAL CATA; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT); CONICYT PIA/BASAL Chilean Ministry for the Economy, Development Premiale VLT 2012 / Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR); Ministry of Education, Universities and Research (MIUR) IC12009 / Tourism's Programa Iniciativa Cientifica Milenio ESF (European Science Foundation) through the GREAT Research Network Programme 188.B-3002 / La Silla Paranal Observatory
- Language
- English
- Date published
- 12/21/2014
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984701824102771
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