Fig. C.3.

Same as Figs. 6 and 7, distribution of relative time differences ΔtKL of falling asteroids in the Roche lobe of the central compact object due to quadrupolar Kozai-Lidov oscillations, for the current Solar asteroid belt (green) and the primordial belt, for an inclination of the outer body hole plane ic = 5° (orange) and ic = 45° (blue), and initial asteroid number Nast = 103. We consider a high mass Mc = 10 M⊙ wide system (left) with ac = 100 AU and ⟨aast⟩ = 1 AU, and a close system (right) with ac = 10 AU and ⟨aast⟩ = 1 AU.
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.