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CCD PHOTOMETRY OF E 1013-477 : AN INTERMEDIATE POLAR SYSTEM ?

The authors have obtained the first I-band CCD photometry of the AM Her candidate E1013-477 in a faint state. There is no evidence for any periodicity near the claimed 103.4-min orbital period. However, they observed significant variability on a time scale of ≡6.4 hrs and a possible period of 71.1 min. The authors therefore propose that E1013-477 may be an intermediate polar system. This interpretation is also consistent with previous observations.