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Resolving Physical Conditions of Diffuse Ionized Gas throughout the Milky Way-Magellanic System
PI Lawrence Haffner
CO-I Edwin Mierkiewicz
We use a dedicated, sensitive spectroscopic facility in Chile, the Wisconsin H-Alpha Mapper (WHAM), to study the physical conditions of the diffuse ionized gas (DIG) in the Milky Way and Magellanic System.
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