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Fig. 11


Age-metallicity distribution for the YOCs we analysed here, for the sample of Netopil et al. (2016) (empty circles), field stars taken from Bensby et al. (2014) (grey crosses), and Gaia-ESO clusters analysed in Magrini et al. (2018) (filled triangles). The red line represents the model by Minchev et al. (2013) for 7.5 < RGal < 9 kpc. See text for further details. The empty stars represent the clusters we analysed whose metallicity was derived with the standard analysis (Netopil et al. 2016).

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