  We examine gravitational waves in an isolated axi--symmetric reflexion
symmetric NGT system. The structure of the vacuum field equations is analyzed
and the exact solutions for the field variables in the metric tensor are found
in the form of expansions in powers of a radial coordinate. We find that in the
NGT axially symmetric case the mass of the system remains constant only if the
system is static (as it necessarily is in the case of spherical symmetry). If
the system radiates, then the mass decreases monotonically and the energy flux
associated with waves is positive.
