Fig. B.2.
Download original image
Orbital evolution during tidal disruption and mass transfer. Top two panels: Semimajor axis and eccentricity evolution of outer planets (1 and 10 M⊕) in the Closer regime. Bottom two panels: Evolution of the remnant core in the Farther regime. Dashed lines mark initial semimajor axes. Eccentricities rise from zero up to ∼0.07 in chaotic configurations.
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.