Kinematics of HD 93840 (full line: adopting the Gaia-based distance $d_{Gaia}^{\text{MA},\text{EB}}$, see Appendix B; dashed: spectroscopic distance d_spec) in the Galactic potential, together with several other runaway stars from our previous work. Galactic Cartesian coordinates XYZ are employed, with the origin shifted to the position of the Sun; ρ is the galactocentric distance. Displayed here: the Galactic plane projection (left panel) and the movement in the meridional plane (right panel). The dots mark the current positions and the orbits are traced back for the stellar age (full lines) and 2 Myr into the future (dotted lines). See the text for a discussion.