Abstract
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) |
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Journal | American Astronomical Society, AAS Meeting #233 |
Volume | 233 |
State | Published - Jan 1 2019 |