Fig. 13
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Age-velocity relation for the MRS and LRS samples coloured by the relative number of stars in each point (divided by the maximum). Power law fitting the 2 < Age < 9 Gyr range are plotted in orange and green dashed lines. A comparison with the AVR obtained for clusters in the solar neighbourhood (Tarricq et al. 2021) is shown in blue dots and their power-law fits in a blue dashed line.
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