  Using a solution-generating method, we derive an exact solution of the
Einstein's field equations in five dimensions describing multi-black hole
configurations. More specifically, this solution describes systems of
non-extremal static black holes with Kaluza-Klein asymptotics. As expected, we
find that, in general, there are conical singularities in-between the
Kaluza-Klein black holes that cannot be completely eliminated. Notwithstanding
the presence of these conical singularities, such solutions still exhibit
interesting thermodynamical properties. By choosing an appropriate set of
thermodynamic variables we show that the entropy of these objects still obeys
the Bekenstein-Hawking law for spaces with Kaluza-Klein asymptotics. This
extends the previously known thermodynamic description of asymptotically flat
spaces with conical singularities to general spaces with Kaluza-Klein
asymptotics with conical singularities. Finally, we obtain a charged
generalization of this multi-black hole solution in the general
Einstein-Maxwell-Dilaton theory and show how to recover the extremal
multi-black hole solution as a particular case.
