  We show that the periodic FRB 180916.J0158+65 can be interpreted by invoking
an interacting neutron star binary system with an orbital period of $\sim 16$
days. The FRBs are produced by a highly magnetized pulsar, whose magnetic field
is ``combed'' by the strong wind from a companion star, either a massive star
or a millisecond pulsar. The FRB pulsar wind retains a clear funnel in the
companion's wind that is otherwise opaque to induced Compton or Raman
scatterings for repeating FRB emission. The 4 day active window corresponds to
the time when the funnel points toward Earth. The interaction also perturbs the
magnetosphere of the FRB pulsar and may trigger emission of FRBs. We derive the
physical constraints on the comb and the FRB pulsar from the observations and
estimate the event rate of FRBs. In this scenario, a lower limit on the period
of observable FRBs is predicted. We speculate that both the intrinsic factors
(strong magnetic field and young age) and the extrinsic factor (interaction)
may be needed to generate FRBs in neutron star binary systems.
