  In this paper we, first, present a class of charged rotating solutions in
four-dimensional Einstein-Maxwell-dilaton gravity with zero and Liouville-type
potentials. We find that these solutions can present a black hole/string with
two regular horizons, an extreme black hole or a naked singularity provided the
parameters of the solutions are chosen suitable. We also compute the conserved
and thermodynamic quantities, and show that they satisfy the first law of
thermodynamics. Second, we obtain the ($n+1$%)-dimensional rotating solutions
in Einstein-dilaton gravity with Liouville-type potential. We find that these
solutions can present black branes, naked singularities or spacetimes with
cosmological horizon if one chooses the parameters of the solutions correctly.
Again, we find that the thermodynamic quantities of these solutions satisfy the
first law of thermodynamics.
