Authorea

How-Huan Hope Chen edited figures/Andre_filament/caption.tex over 9 years ago

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Replace this text with your caption Sketch of the typical velocity field inferred from line observations (e.g., H. Kirk et al., 2013) within and around a supercritical filament (here Serpens-South in the Aquila complex – adapted from Sugitani et al., 2011): Red arrows mark longitudinal infall along the main filament; black arrows indicate radial contraction motions; and blue arrows mark accretion of background cloud material through striations or subfilaments, along magnetic field lines (green dotted lines from Sugitani et al.).