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We present near-infrared and optical emission-line and stellar kinematics ofthe Seyfert 2 galaxy Mrk 573 using the Near-Infrared Field Spectrograph (NIFS)at Gemini North and Dual Imaging Spectrograph (DIS) at Apache PointObservatory, respectively. By obtaining full kinematic maps of the infraredionized and molecular gas and stellar kinematics in a 700 x 2100 pc^2circumnuclear region of Mrk 573, we find that kinematics within the Narrow-LineRegion (NLR) are largely due to a combination of both rotation and in situacceleration of material originating in the host disk. Combining theseobservations with large-scale, optical long-slit spectroscopy that tracesionized gas emission out to several kpcs, we find that rotation kinematicsdominate the majority of the gas. We find that outflowing gas extends todistances less than 1 kpc, suggesting that outflows in Seyfert galaxies may notbe powerful enough to evacuate their entire bulges.

astrophysical journal/the astrophysical journal

Gemini Near Infrared Field Spectrograph Observations of the Seyfert 2  Galaxy Mrk 573: In Situ Acceleration of Ionized and Molecular Gas Off Fueling  Flows