Ionised gas kinematics in MaNGA AGN

We analyse the kinematics of 170 AGN host galaxies as compared to those a matched control sample non-active from MaNGA survey in order characterise and estimate extents Narrow Line Region (NLR) kinematically disturbed region (KDR) by AGN. define observed NLR radius farthest distance nucleus within which both [Oiii]/H\beta [Nii]/H\alpha ratios fall BPT diagram H\alpha equivalent width is required be larger than 3.0\AA. The extent KDR defined hosts shows more gas galaxies. derived [Oiii] line profiles reveal that, on average, most luminous (L[Oiii] > 3.8 * 10^40 erg s^-1) possess higher residual difference between gaseous stellar velocities dispersion their Spatially resolved NLR's KDR's were found 55 46 galaxies, with corrected radii 0.2 < r_KDR,c 2.3 kpc 0.4 r_NLR,c 10.1 kpc, relation two given log = (0.53\pm0.12) + (1.07\pm0.22), respectively. extension corresponds about 30 per cent that NLR. Assuming due an outflow, we have estimated ionised mass outflow rates range 10^-5 \approx 1 Myr^-1, kinetic powers 10^34 s^-1. Comparing power outflows luminosities, they are always below 0.05 L_AGN model threshold for having important feedback effect respective (and power) our correlate populating lowest luminosity correlations previously powerful sources.