  Numerical solutions for asymptotically flat rotating black holes in the cubic
Galileon theory are presented. These black holes are endowed with a nontrivial
scalar field and exhibit a non-Schwarzschild behaviour: faster than $1/r$
convergence to Minkowski spacetime at spatial infinity and hence vanishing of
the Komar mass. The metrics are compared with the Kerr metric for various
couplings and angular velocities. Their physical properties are extracted and
show significant deviations from the Kerr case.
