  This paper is devoted to the study of Hawking radiation as a tunneling of
charged fermions through event horizons of a pair of charged accelerating and
rotating black holes with NUT parameter. We evaluate tunneling probabilities of
outgoing charged particles by using the semiclassical WKB approximation to the
general covariant Dirac equation. The Hawking temperature corresponding to this
pair of black holes is also investigated. For the zero NUT parameter, we find
results consistent with those already available in the literature.
