Fig. 17.

Distributions of filament length (panel a); heliocentric distance (panel b); logarithm of cloud mass Mcloud (panel c); line width Δv (panel d); logarithm of gas surface density Σgas (panel e); logarithm of dense gas mass Mdense (panel f); free-fall time obtained based on spherical morphology (panel g); aspect ratio (panel h); and logarithm of dense gas mass per unit length (panel i).
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