  To help understand the effects of galaxy interactions on star formation, we
analyze Spitzer infrared and GALEX ultraviolet images of the interacting galaxy
pair Arp 82 (NGC 2535/6), and compare to a numerical simulation of the
interaction. We investigate the UV and IR properties of several star forming
regions (clumps). Using the FUV/NUV colors of the clumps we constrain the ages.
The 8 micron and 24 micron luminosities are used to estimate the far-infrared
luminosities and the star formation rates of the clumps. We investigate
possible gradients in the UV and IR colors. See Smith et al. (2006a,b) for
global results on our entire interacting sample.
