Fig. 5

Models for the sub-mm dust emission from the ring system at ALMA Band 7 as a function of mass of the central substellar object using models from Baraffe et al. (2008), together with the ALMA photometry of the point source and the upper limit at the location of the star J1407. Three different disk configurations are presented. Colours correspond to separations from the star J1407: yellow 5 au, orange 10 au, blue 16 au.
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.