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Fig. B.1

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A diagram showing how the probabilistic method should be conceptualised. The radius R = Rboundary − Rcluster. All the stars outside of the cluster are initially assumed to be runaways for the binomial probability problem to calculate the likelihood of multiple alignment events between the runaways and the filaments (grey clouds). The filaments at these scales,  >5 pc, will not be affected by a single O-star such that nothing remains.

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