Maps of the boundedness parameter, b_clumps (top left) and b_regions (bottom left); maps of the star formation efficiency, SFE_clumps (top middle) and SFE_regions (bottom middle); and velocity dispersion, σ_v,clumps (top right) and σ_v,regions (bottom right) of the gas, for the galaxy NGC 7469. The two methods yield comparable results, as evidenced by the spatial distribution of the regions and clumps within the galaxy.