Abstract
Abstract UBVR light curves of the interacting early-type binary system SZ Camelopardalis have been analyzed and compared with model light curves which take into account the influence of anisotropic stellar wind from one of the components. It is indicated that the best fit can be achieved assuming mass transfer from the secondary component with the mass loss rate of 1÷ 5 × 10−TM⊙ /yr.
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Schedule a callMore From: Astronomical and Astrophysical Transactions, Vol. 33, No. 3
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