Fig. 3.
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MZ*R of bulges (red squares) and disks (yellow circles) of CIELO galaxies, defined by median [Fe/H]. For comparison, the CIELO galaxy MZ*R is also included (light blue line). Additionally, observational trends reported by Jegatheesan et al. (2024) for the bulges (red shaded regions) and disks (yellow shaded regions) are also included. Shaded regions are determined by the 16th–84th percentiles.
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