Open Access

Fig. B.1.

image

Download original image

Evolution of the eccentricity for the 3-body PN integration model. Initial positions and velocities were chosen from the full scale N-body model with N = 540k first randomisation at three moments of time in the first ZLK oscillation period from top to bottom: when orbital eccentricity for the inner binary S1+S2 was 0.5, 0.7 and 0.9. We individually turned “on” the different combination of PN terms in our 3-body PN code: PN0 (“Newtonian”), PN0+PN1, PN0+PN1+PN2, only PN0+PN2.5 and PN-Full = PN0+PN1+PN2+PN2.5 (i.e. with “Full”).

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.