Press Release
Free Access

Fig. 13.


Spectra of individual clumps #1.2 S (left panel) and #1.2 N (right panel), extracted from our PdBI CO(4–3) data cube using 0.6″ × 0.6″ apertures, and corrected for gravitational magnification. Clump #1.2 N is well fitted with a single Gaussian function (red curve), while #1.2 S exhibits a secondary component, blueshifted with respect to the systemic component (blue curves), which we interpret as the signature of a stellar wind.

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.