Matt Haffner
Senior Scientist
Email: .(JavaScript must be enabled to view this email address)
Ph: (608) 262-3052
Office: 5514 Sterling Hall
Research Interests:
I am broadly interested in many facets of the structure of the Milky Way, especially the interplay between the gaseous and stellar components. My current efforts are focused on characterizing the Warm Ionized Medium of our ISM with the Wisconsin H-Alpha Mapper (WHAM), currently located at CTIO in Chile.
My Publications
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Photoionization of High-altitude Gas in a Supernova-driven Turbulent Interstellar Medium
Wood, K., Hill, A., Joung, M., Mac Low, M., Benjamin, R., et al., 2010
The Astrophysical Journal, Vol. 721, Pages 1397-1403
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Ionized Gas in the Smith Cloud
Hill, A., Haffner, L., Reynolds, R., 2009
The Astrophysical Journal, Vol. 703, Pages 1832-1838
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The warm ionized medium in spiral galaxies
Haffner, L., Dettmar, R., Beckman, J., Wood, K., Slavin, J., et al., 2009
Reviews of Modern Physics, Vol. 81, Pages 969-997
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The Turbulent Warm Ionized Medium: Emission Measure Distribution and MHD Simulations
Hill, A., Benjamin, R., Kowal, G., Reynolds, R., Haffner, L., Lazarian, A., 2008
The Astrophysical Journal, Vol. 686, Pages 363-378
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