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J.C. Smith, R.D. Dietz (U. of Northern Colorado), M.C. Smith (Front Range C. C.)
We present four-color CCD photometry of U Geminorum covering a nine-hour (2.1 periods) interval obtained twelve days before the February 2004 outburst. The light curves in B,V, and R show a single maximum and are consistent with published results. The I-band light curve exhibits a secondary maximum 0.1 mag fainter than the primary maximum. We discuss possible explanations for this observation.
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Bulletin of the American Astronomical Society, 36 #2
© YEAR. The American Astronomical Soceity.