  We consider rotating Lorentzian wormholes with a phantom field in five
dimensions. These wormhole solutions possess equal angular momenta and thus
represent cohomogeneity-1 configurations. For a given size of the throat, the
angular momenta are bounded by the value of the corresponding extremal
Myers-Perry black hole, which represents the limiting configuration. With
increasing angular momenta the throat becomes increasingly deformed. At the
same time, the violation of the null energy condition decreases to zero, as the
limiting configuration is approached. Symmetric wormhole solutions satisfy a
Smarr-like relation, which is analogous to the Smarr relation of extremal black
holes. A stability analysis shows that the unstable mode of the static
wormholes solutions vanishes when the angular momentum exceeds some critical
value.
