  We consider the classical equations of the Einstein-Yang-Mills model in five
space-time dimensions and in the presence of a cosmological constant. We assume
that the fields do not depend on the extra dimension and that they are
spherically symmetric with respect to the three standard space dimensions. The
equations are then transformed into a set of ordinary differential equations
that we solve numerically. We construct new types of regular (resp. black
holes) solutions which, close to the origin (resp. the event horizon) resemble
the 4-dimensional gravitating monopole (resp. non abelian black hole) but
exhibit an unexpected asymptotic behaviour.
