  We study the classical solutions of the Einstein-Yang-Mills model in five
dimensions in the presence of a cosmological constant $\Lambda$. Using a
spherically symmetric ansatz and assuming that the fields do not depend on the
extra dimension, we transform the equations into a set of 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)
and study their global properties.
