Velocity structure of the C¹⁸O(2–1) emission in L1495/B213. Top: C¹⁸O(2–1) spectra from selected positions illustrating the presence of multiple velocity components along the line of sight. The selected positions are indicated with red circles in the maps below. Bottom: maps of C¹⁸O(2–1) emission integrated in two velocity intervals that approximately coincide with the components in the top spectra. All maps have the same physical scale, color code (shown in the B7/L1495 panel), and contour scale (first contour and interval are 0.3 K km^-1). Coordinate centers and star symbols as in Fig. 2.