A class of exact solutions of Einstein's equations is analyzed which descri
bes uniformly accelerating charged black holes in an asymptotically de Sitt
er universe. This is a generalization of the C metric which includes a cosm
ological constant. The physical interpretation of the solutions is facilita
ted by the introduction of a new coordinate system for de Sitter space whic
h is adapted to accelerating observers in this background. The solutions co
nsidered reduce to this form of the de Sitter metric when the mass and char
ge of the black holes vanish.