Kat Barger

Graduate Student

Email: .(JavaScript must be enabled to view this email address)
Ph: (608) 358-9936
Office: 5510 Sterling

Research Interests:

I'm interested in how galactic interactions with warm halo gas affect galaxy evolution. I study the poorly understood warm ionized gas in the Magellanic System and in High Velocity Clouds.

CV (PDF)

Biography:

My dissertation concentrates on galactic interactions with warm halo gas. Halo gas interactions influence galactic evolution by fueling star formation and modifying metallicity. For this work, I use the Wisconsin Hα Mapper to study the faint, warm ionized gas. The Hα observations allow us to study the extent and large-scale velocity structure of the ionized gas, giving clues on the source(s) of ionization, the ionization fraction, and the mass of the ionized component. In addition, [SII] and [NII] studies probe the physical conditions of these regions, including temperature and metallicity.

The Magellanic System exhibits some of the nearest examples of interactions affecting galaxy...read more

My Publications

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