Left: position of MBM12 relative to the galactic disk. The colour scale shows the Planck 857 GHz dust continuum, and the contours are the neutral hydrogen column density with contours at levels [1.0, 1.2, 1.4] ×10²¹ cm⁻² from the HI4PI all sky survey (HI4PI Collaboration 2016). The beam sizes of Planck 857 GHz (orange) and H14PI (white) are shown in the bottom left. Assuming a distance of 252 pc to MBM12 and a solar height of 20 pc above the galactic plane, the distance of MBM12 from the galactic plane is shown in white. Right: zoom-in of MBM12 with the positions of T Tauri stars from Meeus et al. (2009) shown with cyan [×] markers. The observing field of view of the TRAO and Herschel observations used in this work are shown in white and yellow, respectively. A distance scale is shown in the bottom right.