  The presence of non-circular and off-plane gas motions is frequently observed
in the inner regions of disk galaxies. We have measured with integral-field
spectroscopy the surface-brightness distribution and kinematics of the ionized
gas in NGC 2855 and NGC 7049. These two early-type spiral galaxies were
selected to possibly host a kinematically-decoupled gaseous component in
orthogonal rotation with respect to the galaxy disk. We have modeled the
ionized-gas kinematics and distribution of both galaxies assuming that the
gaseous component is distributed either on two orthogonally-rotating disks or
in a single and strongly warped disk. In both galaxies the velocity field and
distribution of the inner gas are consistent with the presence of an inner
polar disk. In NGC 2855 it correponds to the innermost and strongly warped
portion of the main disk. In NGC 7049 it is a central and
geometrically-decoupled disk, which is nested in the main disk.
