  We construct new black hole solutions in Einstein-Yang-Mills theory. They are
static, axially symmetric and asymptotically flat. They are characterized by
their horizon radius and a pair of integers (k,n), where k is related to the
polar angle and n to the azimuthal angle. The known spherically and axially
symmetric EYM black holes have k=1. For k>1, pairs of new black hole solutions
appear above a minimal value of n, that increases with k. Emerging from
globally regular solutions, they form two branches, which merge and end at a
maximal value of the horizon radius. The difference of their mass and their
horizon mass equals the mass of the corresponding regular solution, as expected
from the isolated horizon framework.
