Signatures of UV radiation in low-mass protostars - I. Origin of HCN and CN emission in the Serpens Main region

Open Access

Fig. 4

Emission in the line wings of HCN 1–0, CN 1–0, CS 3–2, and CO 6–5 toward Ser SMM1 (blue and red contours). The velocity ranges used to calculate the integrated intensities are provided in Appendix D. The black and green lines correspond to outflow directions in CO 3–2 and CO 6–5 (as in Fig. 2).

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.