Maps of the clouds properties (see Sect. 3.3). The panels show a sum of the window function weights, Σ_iw_i (a), weighted medians for the nearest neighbour separation, r_nnb (b), and the absolute value of the nearest neighbour velocity, v_nnb (c), and the probability of finding clouds with properties more extreme than those in a given point (d). The corresponding zooms into 30Dor are shown in the upper right corners of each individual map. The majority of low-probability “spots” in panel d are visually associated with known active star formation regions in the LMC (N158, N159, etc.), except for one spot marked by the yellow box.