Figure 10
From: A new hybrid technique for modeling dense star clusters
Properties of Ejected Binary BH systems—The properties of the ejected binary BH systems from each of the four NBODY6 models (black diamonds) and from the 10 RAPID realizations (red circles). We show the eccentricity and semi-major axis (in AU, assuming each cluster to have an initial virial radius of 1 parsec) for each binary. In each case, the NBODY6 results align with the larger sample size from the RAPID models. The text in each plot indicates the total number of ejected binaries from the NBODY6 models, and the mean and standard deviation from the 10 RAPID models