  Quasinormal modes of a scalar field perturbation are investigated in the
background spacetime of Einstein-Yang-Mills black holes. The logarithmic term
in the metric function of the five-dimensional Einstein-Yang-Mills black hole
eliminates the divergence of the Hawking temperature but maintains the
charge-dependent behavior of the quasinormal modes. The real and imaginary
parts of quasinormal mode frequencies have the same charge-dependent behavior
in different dimensions. Similar to the case of high dimensional Schwarzschild
black holes, a compact approximate relation, $\omega_{\rm R}\sim D/r_{+}$, also
exists between the real part of the quasinormal mode frequencies $\omega_{\rm
R}$ and the number of dimensions $D$ in the higher than five dimensional
Einstein-Yang-Mills black holes.
