Fig. 18
All measured transverse velocities of binary radio pulsars with a WD companion. Data taken from the ATNF Pulsar Catalogue in March 2013 (Manchester et al. 2005 http://www.atnf.csiro.au/research/pulsar/psrcat). AIC is expected to form binary pulsars with v⊥ < 30km s-1. However, the observed binary pulsars with such small velocities could also have formed by EC SNe.
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