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Fig. 3.

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Number of living 4 M HVSs as a function of the time of observation. The ejection begins at t = 0 with a rate 10−4 yr−1. The number of living HVSs stops increasing beyond t ≃ τL = 160 Myr. The vertical dashed line marks the time of the steady state when we chose to observe the system, tobs = 400 Myr.

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