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Open clusters in the Gaia-ESO Survey: tracing the chemical history of the Milky Way thin disk

Published online by Cambridge University Press:  17 July 2015

L. Magrini  and
S. Randich
L. Magrini
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
S. Randich
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Florence, Italy
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Abstract

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that aims at observing with FLAMES@VLT the main stellar components of our Galaxy. The study of the population of open clusters is one of the main objectives of GES. We present some results from the first 18 months of observations, among them, a preliminary view of the radial metallicity gradient as traced by open cluster data and a comparison of the chemical patterns of clusters located in different parts of the Galactic disk.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 68: The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases , 2014 , pp. 115 - 122
Copyright
© EAS, EDP Sciences, 2015

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