Fig. 6
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Dependence of the orbital parameters zmax (top) and eccentricity (bottom) on the age and galactocentric radius of OCs. In the top panel, we fit the data with an exponential function. Objects observed with MEGARA are marked with circles, and objects observed with OCCASO (Carrera et al. 2022) are shown as triangles. In all of them, the galactocentric radius is colour-coded.
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