Fig. 5
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[C/H] chemical inhomogeneities in the Galactic disc for samples A and C. Left panel: map of [Ca/H] excess for sample A, including the spiral arm contours from Poggio et al. (2021) adopting the same local bandwidth as for [Ca/Fe]. Right panel: same for sample C, including the spiral arm contours from Palicio et al. (2023) adopting the same local bandwidth as for [Ca/Fe].
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