Clayton Hogen-Chin

University of Minnesota
Department of Astronomy

My research is on the infrared polarization of the edge-on spiral galaxy NGC3628. Polarization of infrared radiation is partly caused by the alignment of dust grains within the galactic magnetic field, and so can be used to trace that field. By looking at the polarization around the core of NGC3628 we hope to better understand the effects of the AGN on the galactic magnetic field.

The Roof of Africa - Mt. Kilimanjaro (19336 ft)

email me