WISE RGB images in W4+W3+W2 for the known bow shock and bubble candidates presented in Table 5 in equatorial coordinates, with north up and east to the left. Dashed white arrows indicate the directions of the original proper motions from Gaia DR3, and solid cyan arrows indicate the directions of the proper motions corrected for the ISM motion caused by Galactic rotation. Each field has a different size, but the arrows are fixed to 2′. Each panel contains the name of the star as provided in the GOSC or the BeSS catalogs, and the runaway star id.