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M. La Vigne (WMC), J. S. Shaw (UGA)
We present preliminary solutions for BVRI light curves of the eclipsing binary stars Aur0 4982 and a newly discovered variable. Aur0 4982 is a detached system with a spot on its cooler, less massive star. The new variable system is semi-detached with the cooler, less massive star filling its Roche lobe. We have determined a new period for both Aur0 4982 and the new variable. The National Science Foundation supported this work through their Research Experience for Undergraduates grant AST-0097616.