Description of turbulent dynamics in the interstellar medium: Multifractal microcanonical analysis - II. Sparse filtering of Herschel observation maps and visualization of filamentary structures at different length scales

Open Access

Fig. 13

Aquila flux intensity map from Herschel at 250 μm. We show a zoom onto one subregion where the flux intensity is more intense (W40 subregion).

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