Velocity distributions for VFTS 243 and its host association. The measured velocity components for VFTS 243 (red), compared to the inferred dispersion of its birth association, the Tarantula nebula (blue, arbitrary scaling), estimated from the massive binaries in the TMBM survey. From top to bottom, the panels show the velocity in the direction of increasing RA and in the direction of increasing Dec and in the radial direction. For the Tarantula dispersion, a 90% credible interval of the inferred distributions is shown.