Formation and evolution of the two 4/3 resonant giants planets in HD 200964

Free Access

Fig. 8

Open with DEXTER Download original image

The 4/3 resonance stable ACRs parameterized by the mass ratio m₂/m₁. The family with the mass ratio 0.45 corresponding to the simulated HD 200964 system (Table 1, last column) is shown by a red curve. The crosses are ACR whose neighborhood was analyzed and whose stability maps are shown in Fig. 9.

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.