Fig. B.2
Download original image
Comparison of the computed masses (upper panel) and column densities (lower panel) for selected clumps in NGC 6334 to the values derived by Urquhart et al. (2018) for the same clumps. The Pearson correlation coefficient, R, and the P value are given in the lower-right and upper-left corner, respectively, where also the fitted linear relations are indicated.
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.