Angular offsets of the pulsars with published timing solutions from the centres of their clusters, in core radii. The larger the encounter rate per binary γ, the larger are the odds of finding pulsars far from the centres of their clusters. Some of the clusters are labelled as in Table 1, colours are used to discriminate isolated and binary pulsars, and symbols to indicate the companion mass. Binaries created by exchange products are shown light blue. The dashed line indicates a distance of 4 core radii.