Fig. 12
Comparison of the effective temperature distribution of intrinsic (upper panel) and extrinsic (lower panel) S stars collected from Table 4. The dashed line indicates the subset of stars falling in the metallicity bin (−0.75 < [Fe/H] ≤ −0.25), while the shaded histogram concerns stars within the −0.25 < [Fe/H] ≤ 0.25 solar metallicity bin.
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