Free Access

Fig. 5

thumbnail

Examples of integration runs for the HD 196885 3 body system. The evolution of the inner orbit Ab is shown over 107   yr. Top: a typical coplanar solution, with semi-major axis (left) and eccentricity (right) evolution; Bottom: same for a typical highly ir solution with kozai oscillations (see eccentricity).

This figure is made of several images, please see below:

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.