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Radiation transfer in a sphere with internal source
Authors:E A Saad  S A El Wakil
Institution:(1) Department of Astronomy, University of Cape Town, South Africa
Abstract:From the presence of superhumps in its outburst light curve, the dwarf nova BR Lup is shown to be a member of the SU UMa sub-class of cataclysmic variables. Its orbital period is estimated to be 0.0789 d.
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