Fig. 4.
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Chemical abundance patterns for the Terzan 6 stars observed with X-shooter (filled triangles) and NIRSpec (open squares). Typical error bars for the [Fe/H] and [X/Fe] abundance ratio values are also plotted in the corner of each panel. For comparison, the corresponding measurements of giant stars (dots) in other bulge GCs (see Origlia et al. 2008; Valenti et al. 2011, and references therein) are also reported.
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