  We derive a correspondence between the Hawking radiation spectra emitted from
general classes of Taub-NUT black holes with that induced by the relativistic
motion of an accelerated Dirichlet boundary condition (i.e.\ a perfectly
reflecting mirror) in (1+1)-dimensional flat spacetime. We demonstrate that the
particle and energy spectra is thermal at late-times and that particle
production is suppressed by the NUT parameter. We also compute the radiation
spectrum in the rotating, electrically charged (Kerr-Newman) Taub-NUT scenario,
and the extremal case, showing explicitly how these parameters affect the
outgoing particle and energy fluxes.
