The Gaia-ESO Survey: Metallicity of the Chamaeleon I star-forming region
Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun and older clusters in the solar vicinity. However, these results are based on small statistics and inhomogeneous analyses. The Gaia-ESO Survey is observing and
Spina, L. et al.
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2014