Free Access

Fig. A.3


Eccentricity as a function of semimajor axis for a planetary system orbited by a secondary star of 1 M after 0.5 Myr of integration using Nemesis (big black bullets) and the single 8th order symplectic integrator in Huayno (smaller white bullets). The final eccentricity of the planets in the direct integration and the component method are indistinguishable in the figure, with an absolute mean error < 2 × 10−4 for each of the planets.

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.