Fig. 2
Cut through the Herschel/PACS images along the belt’s major axis on the sky. The surface brightness profiles are normalized by the maximum values indicated in Table 1. The off-center position of the star is indicated. The belt’s peak positions are located closer to the belt center at 160 μm, which is a consequence of the reduced angular resolution (see Sect. 2.2).
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.