Open Access

Fig. 7

image

Probability of the pair d–c to be Hill-stable as a function of the mutual inclination of d and c, assuming planet b is within the invariant plane. The masses, semi-major axes, and eccentricity are drawn from the best-fit distribution (Christiansen et al. 2017). The dashed curve corresponds to a system where every planet is on a circular orbit.

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.