Pericenter precession induced by a circumstellar disk on the orbit of massive bodies: comparison between analytical predictions and numerical results

Free Access

Fig. 3

Open with DEXTER Download original image

Comparison between the disk force for p = 1 and R_in = 0.5 AU. Both F^W and F^SR almost perfectly match the numerical values even close to the star, showing the relevance of including an inner cutoff of the disk at R_in.

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.