Gas kinematics around filamentary structures in the Orion B cloud

Open Access

Fig. 3

Mean spectra of the three layers of the Orion B cloud, namely the low-velocity layer (left), the intermediate-velocity layer (middle), and the main-velocity layer (right), from the ¹³CO (1–0) (top) and C¹⁸O (1–0) (bottom) emission rebuilt by ROHSA. The color dotted lines show the systemic LSR velocity of the three cloud layers.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.