  In previous papers, we have proposed a model that the high-frequency
quasi-periodic oscillations (HF QPOs) observed in black-hole and neutron-star
X-ray binaries are inertial-acoustic oscillations that are resonantly excited
on a one-armed deformed disk by nonlinear couplings between the oscillations
and the disk deformation. In this paper we show that in addition to the
inertial-acoustic waves, one-armed corrugation waves are also excited in the
deformed disks. They are low-frequency oscillations. We examine frequencies and
their correlations among the inertial-acoustic oscillations and the corrugation
waves that are excited, in order to know whether they can describe observed
frequency correlations among kHz QPOs and low-frequency QPOs (LF QPOs) in
neutron-star X-ray binaries. The results seem to well describe the observed
correlations in Cir X-1, if we adopt $M= 1.5\sim 2.0 M_\odot$ and $a_* \sim
0.8$, where $M$ is the mass of the central star and $a_*$ is the dimensionless
spin parameter of the metric. Finally, assumptions involved in this
disk-oscillation model are briefly summarized and discussed.
