A class of exact solutions of the Einstein–Maxwell equations is presented which describes an accelerating
and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe.
The metric is presented in a new and convenient form in which the meaning of the parameters is
clearly identified, and from which the physical properties of the solution can readily be interpreted.
This is a pre-print. It is also available at: http://xxx.soton.ac.uk/abs/gr-qc/0601130.