Open Access

Fig. 9.

image

Download original image

Post-disruption orbital eccentricities, e, for a star of mass 1 M (left) and 0.5 M (right) initially in a parabolic orbit, due to a BH of mass 10 M (top) and 40 M (bottom) and as a function of impact parameter b and MS age (Hc abundance). The dashed line represents parabolic orbits and separates the parameter space into bound (eccentric) and unbound (hyperbolic) orbits. The reason for the trends is the same as that for Fig. 8.

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.