Free Access
Fig. 13
Ratios of the CO 10–9/3–2 line wings for 14 protostars as function of velocity offset from the central emission. Spectra are shifted to Vlsr = 0 km s-1. The wings start at ±2.5 km s-1 from Vlsr in order to prevent adding the central self-absorption feature in the CO 3–2 lines.
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.