Fig. 3
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Evolution of Jacobi mass, MJ, and ratio of half-mass radius to Jacobi radius, λ, as a function of age. Top panel: MJ for the BFSR (blue) and the COSR (red). Bottom panel: λ for the BFSR (blue) and the COSR (red). The observed values at 708 Myr are marked with a black cross. The data of the BFSR are shown until the cluster dissolves after 1.53 Gyr.
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