  We present long slit spectroscopy for the [OIII] and H$\alpha$ wavelength
ranges along nine different position angles for the Sa Seyfert 1.9 galaxy NGC
2992. Double profiles are present in several regions, suggesting that the gas
is not simply following galaxy rotation. A simple kinematical model, which
takes into account circular rotation together with a constant radial outflow,
seems to be a good approximation to account for the observed kinematics.
