  More than 100 radio pulsars have been detected in 24 globular clusters. The
largest observed samples are in Terzan 5 and 47 Tucanae, which together contain
45 pulsars. Accurate timing solutions, including positions in the cluster, are
known for many of these pulsars. Here we provide an observational overview of
some properties of pulsars in globular clusters, as well as properties of the
globular clusters with detected pulsars. The many recent detections also
provide a new opportunity to re-examine theoretically the formation and
evolution of recycled pulsars in globular clusters. Our brief review considers
the most important dynamical interaction and binary evolution processes:
collisions, exchange interactions, mass transfer, and common-envelope phases.
