ИСТИНА

In the project we are investigating the generation of large scale outflows in galaxies. We are combining optical integral-field spectroscopy data from the MaNGA survey with, sensitive, high-resolution (compatible with optical data ~1’’) radio (Jansky Very Large Array; JVLA) observations for sample of 30 galaxies with high-velocity components in the [OIII] emission line, which includes AGN, starbursts and composite sources. In this talk, we will present a case study of two galaxies where AGN are thought to drive the outflow. Despite a common origin, we find a dichotomy in the AGN behavior: the galaxy with a more luminous AGN powers a weaker outflow with no corresponding radio emission, while the galaxy with a weaker AGN powers a more powerful outflow coincident with a radio jet. Furthermore, analysis of the optical morphology of both galaxies suggest both have recently interacted with a neighbor, possibly triggering their AGN activity.