  We investigate theoretically Fermionic superfluidity induced by Feshbach
resonance in the orbital p-wave channel. We show that, due to the dipole
interaction, the pairing is extremely anisotropic. When this dipole interaction
is relatively strong, the pairing has symmetry $k_z$. When it is relatively
weak, it is of symmetry $k_z + i \beta k_y$ (up to a rotation about $\hat z$,
here $\beta < 1$). A phase transition between these two states can occur under
a change in the magnetic field or the density of the gas.
