Fig. 8.

Fraction of mass accreted by the companion as a function of v∞/vorb. The dotted line corresponds to BHL accretion rate with BHL = 1, and the dashed line to the accretion rate for a geometrical cross section of size Rsink. Dots correspond to models in which the orbital separation is 5 AU and stars to models in which a = 3 AU. The values shown are measured at a radius of 0.4 RL,2 (β0.4RL,2).
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