  We present near-infrared and optical emission-line and stellar kinematics of
the Seyfert 2 galaxy Mrk 573 using the Near-Infrared Field Spectrograph (NIFS)
at Gemini North and Dual Imaging Spectrograph (DIS) at Apache Point
Observatory, respectively. By obtaining full kinematic maps of the infrared
ionized and molecular gas and stellar kinematics in a 700 x 2100 pc^2
circumnuclear region of Mrk 573, we find that kinematics within the Narrow-Line
Region (NLR) are largely due to a combination of both rotation and in situ
acceleration of material originating in the host disk. Combining these
observations with large-scale, optical long-slit spectroscopy that traces
ionized gas emission out to several kpcs, we find that rotation kinematics
dominate the majority of the gas. We find that outflowing gas extends to
distances less than 1 kpc, suggesting that outflows in Seyfert galaxies may not
be powerful enough to evacuate their entire bulges.
