Fig. 3
Polaris column density map derived from Herschel imaging data taken as part of the HGBS and “Evolution of interstellar dust” key programs. The brightest structure with the highest column density value located on the south-western part of the field has been labelled as MCLD 123.5+24.9 and as the “saxophone” by Schneider et al. (2013).
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.