Fig. 5.
Abundance pattern of F3D GCs. [Fe/H] in relation to [α/Fe] (left) and [M/H] (right). Right panel: the grey crosses show the distribution for the MILES stars that were used to construct the E-MILES models and the purple line is a least-square fit with a piecewise linear function (Eq. (3)) to the MILES stars. The cyan circles show the brightest F3D GCs in our sample.
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