Fig. 6
Top: median SFD of the impactors on Ceres and Vesta, coming from the different source regions of the MB, derived from the second selection of runs. The large end of this SFD, when D > 10−20 km, must behandled with care due to the high stochasticity of big impact events and small numbers. Bottom: relative contribution from each region of the MB to the impactors in the range 0.1− 10 km, with respectto the total cumulative number of impacts.
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