Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs

We explore the relationship between the ionized gas outflows and radio activity using a sample of similar to 6000 active galactic nuclei (AGNs) at z < 0.4 with the kinematical measurement based on the [O III] line profile and the radio detection in the VLA FIRST Survey. To quantify radio activity, we divide our sample into a series of binary subclasses based on the radio properties, i.e., radio luminous/radio weak, AGN-dominated/star-formation contaminated, compact/extended, and radio loud/radio quiet. None of the binary subclasses exhibits a significant difference in the normalized [O III] velocity dispersion at a given [O III] luminosity once we correct for the influence of the host galaxy's gravitational potential. We only detect a significant difference in [O III] kinematics between the high and low radio-Eddington ratio (L-1.4 GHz/L-Edd) AGNs. In contrast, we find a remarkable difference in ionized gas kinematics between high and low bolometric-Eddington ratio AGNs. These results suggest that accretion rate is the primary mechanism in driving ionized gas outflows, while radio activity may play a secondary role providing additional influence on gas kinematics.