Can we characterize "hub" clumps vs "filament" clumps by examining their azimuthal column density profile? Filaments would have two-peaked structures, hubs many-peaked, and spherically symmetric "isolated" clumps would be peakless.
Can we characterize "hub" clumps vs "filament" clumps by examining their azimuthal column density profile? Filaments would have two-peaked structures, hubs many-peaked, and spherically symmetric "isolated" clumps would be peakless.