Large scale outflows from galaxies are typically associated with AGN or star formation activity however it's still unclear how these outflows are generated and how the properties of the outflow are connected to their origins or their hosts. This requires measuring the spatially-resolved properties of the outflow and its host galaxy in multiple wavebands, in order to measure relevant parameters such as level of AGN galactic, rate and distribution of star formation, and geometry, content, and velocity of the outflow. To this end, we will present detailed analysis of the spatially-resolved radio and optical emission of two SDSS-IV MaNGA outflow galaxies.
|Original language||English (US)|
|Journal||American Astronomical Society, AAS Meeting #233|
|State||Published - Jan 1 2019|