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Fig. A.10
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GRK velocity, vGRk, versus mass ratio, q, of the participating compact objects. All but one event are BHBH mergers; the exception is a BHNS merger, marked by an extreme q and low vGRk. The shaded part of the plot corresponds to the interval 26.9 - 159.4 km s−1, the escape speeds range in cluster cores among all models.
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