Fig. 10.

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Abundance ratios [Mg/Fe], [Si/Fe], [Ca/Fe], [Ti/Fe]I, and [Ti/Fe]II for stars in NGC 6388 as a function of the effective temperature. For the present work, red filled circles indicate stars with GIRAFFE spectra, whereas stars with UVES spectra are represented with blue filled squares. Large black circles indicate the four stars analysed by Minelli et al. (2021a), and green filled triangles are stars in APOGEE DR17 flagged as members of NGC 6388.
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