  We investigate the nonlinear behaviour of the dynamically unstable rotating
star for the bar mode by three-dimensional hydrodynamics in Newtonian gravity.
We find that an oscillation along the rotation axis is induced throughout the
growth of the unstable bar mode, and that its characteristic frequency is twice
as that of the bar mode, which oscillates mainly along the equatorial plane. A
possibility to observe Faraday resonance in gravitational waves is demonstrated
and discussed.
