Fig. 10.
Mean LTE metallicities and [Mg/Fe] and [Ti/Fe] abundance ratios for all clusters and for Milky Way field stars from Bensby et al. (2014) (NLTE [Fe/H], LTE [Mg/Fe] and LTE [Ti/Fe] – small dots) and Bergemann et al. (2017b) (1D LTE results – small crosses). Error bars represent the 1σ intra-cluster abundance variations. Colours are the same as in Fig. 9.
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