Fig. 9
Binary mutual orbit inclination against semimajor axis relative to the Hill radius, recreated from Fig. 1 of Grundy et al. (2019). We overplot the binary systems from our simulations using the same marker shapes and colours as in Fig. 2 to represent the cloud mass. As in Fig. 8, the larger bold points highlight the observable binary systems and the observed TNBs are black crosses.
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