Free Access

Fig. 5


Fourier analysis of the surface density of all non self-gravitating Kepler-16 circumbinary disks. The transform is done on the time-averaged surface density, over a single binary orbit at 15 000 PAB, to consider only l = 0. The strengths of both the m = 1 and m = 2 modes are normalised against the axisymmetric (m = 0) contribution and plot as a function of radius in the disk.

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.