B. Dębski, L. Kulczycka, W. Skrobacz, J. Pęgiel, M. Jacak
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Abstract
. We present solutions of the BVRI-light curve numerical modeling for five low-mass ratio totally eclipsing contact binary stars. One object required the introduction of a cool star spot to the best-fitting model. Only one object returned a solution with a hotter secondary component. None of the objects required the introduction of a third component.
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