Zoom-in of the F-star pore-like structure in Fig. 1 showing umbral-dot-like features. Bolometric intensity of the zoomed-in region (left) with vertical cuts in convective velocity, v_z (middle), and the vertical magnetic field, B_z (right), along the y and x axes. The dashed colored lines represent the locations of the cuts and the solid green line represents the τ = 1 surface. The bottom of the simulation box corresponds to z = 0 for reference.