  In this paper, we study the shadow produced by rotating black holes with
charge in the presence of an anisotropic matter field. We obtain the apparent
shape and the corresponding observables characterizing the size, oblateness,
and deviation of the center, for different values of the parameters of the
model. We compare the new results with those corresponding to the Kerr-Newmann
spacetime and we also discuss the observational prospects in this case.
