Fig. 11
Distribution of core-to-filament separations in the Ophiuchus cloud, for both prestellar cores and (unbound) starless cores. For each core, the projected separation to the nearest filament in the sample of filamentary structures extracted with DisPerSE (cf. Sect. 4.3) was considered. For comparison, the red dashed curve shows an example of anormalized, crest-averaged radial column density profile for a filament traced with DisPerSE in Ophiuchus.
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