Image Details
Caption: Figure 8.
The velocity channel maps of C18O (1–0) emission in relation to the identified filamentary structures. The velocity ranges of integration are indicated in the bottom of each panel. The filament spines covering the velocity channel range of each panel are overlaid with the same colors as the ones for the filaments in Figure 7.
© 2023. The Author(s). Published by the American Astronomical Society.