  It is known that NUT solution has many interesting features and pathologies
like being non-singular and having closed timelike curves. It turns out that in
higher dimensions horizon topology cannot be spherical but it has instead to be
product of $2$-spheres so as to retain radial symmetry of spacetime. In this
letter we wish to present a new solution of pure Gauss-Bonnet $\Lambda$-vacuum
equation describing a black hole with NUT charge. It has three interesting
cases: (a) black hole with both event and cosmological horizons with
singularity being hidden behind the former, (b) a regular spacetime free of
both horizon and singularity, and (c) black hole with event horizon without
singularity and cosmological horizon. Singularity here is always non-centric at
$r \neq 0$.
