Fig. A.2
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Total number of predicted stars (N★) as a function of the Galactocentric distance and the Galactic time. Upper panel: Results from the reference model without including stellar migration. Middle panel: Results from the model incorporating stellar migration, as described in Section 2.2, with the radial migration strength fixed at σRM = 3.5. Lower panel : Same as the middle panel but with a radial migration strength of σRM = 6. In each panel, we highlight with a green cross the maximum number of stars computed at 12 kpc.
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