  We investigate static axially symmetric black hole solutions in a
four-dimensional Einstein-Yang-Mills-SU(2) theory with a negative cosmological
constant $\Lambda$. These solutions approach asymptotically the anti-de Sitter
spacetime and possess a regular event horizon. A discussion of the main
properties of the solutions and the differences with respect to the
asymptotically flat case is presented. The mass of these configurations is
computed by using a counterterm method. We note that the $\Lambda=-3$
configurations have an higher dimensional interpretation in context of $d=11$
supergravity. The existence of axially symmetric monopole and dyon solutions in
a fixed Schwarzschild-anti-de Sitter background is also discussed. An exact
solution of the Einstein-Yang-Mills equations is presented in Appendix.
