Fig. 21.

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Same as Fig. 19 for V, Mn, Co, and Cu. The black squares are bulge GC stars from Ernandes et al. (2018), and black crosses show bulge field stars from Ernandes et al. (2020). The chemodynamical evolution models are shown in different radius ranges: r < 0.5 kpc (dash-dotted line), 0.5 < r < 1 kpc (dashed line), 1 < r < 2 kpc (dotted line), and 2 < r < 3 kpc (solid line).
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