Fig. D.1.
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as a function of 
for the simulated runaway stars represented in blue for one of the 10000 simulations that match the GOSC-Gaia DR3 results. The (VTAN,WRSR) velocities of the field stars of the GOSC-Gaia DR3 catalog are depicted in black. Top: Simulated 2D runaway stars. Bottom: Simulated 3D runaway stars with either positive or negative values of 
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