2019MNRAS.489.4111S

We present two-dimensional ionized gas and stellar kinematics in the inner 1.4 x 1.9 kpc² of the Seyfert 2 galaxy ESO 153-G20 obtained with the Gemini-South/Gemini multi-object spectrograph integral field unit (GMOS-IFU) at a spatial resolution of ∼250 pc and spectral resolution of 36 km s^–1. Strong [O III], Hα, [N II] and [S II] emission lines are detected over the entire field of view. The stellar kinematics trace circular rotation with a projected velocity amplitude of ±96 km s^–1, a kinematic major axis in position angle of 11°, and an average velocity dispersion of 123 km s^–1. To analyse the gas kinematics, we used aperture spectra, position-velocity diagrams and single/double Gaussian fits to the emission lines. All lines show two clear kinematic components: a rotating component that follows the stellar kinematics, and a larger-dispersion component, close to the systemic velocity (from which most of the [O III] emission comes), mainly detected to the south-west. We interpret this second component as gas outflowing at ∼400 km s^–1 in a compact (300 pc) ionization cone with a half-opening angle <=40°. The counter-cone is probably obscured behind a dust lane. We estimate a mass outflow rate of 1.1 M_☉ yr^–1, 200 times larger than the estimated accretion rate on to the supermassive black hole, and a kinetic to radiative power ratio of 1.7 x 10^–3. Bar-induced perturbations probably explain the remaining disturbances observed in the velocity field of the rotating gas component.