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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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We report the results of the analysis of the brightness variability of WZ Sagittae in the beginning of it's relaxation after superoutburst in 2001. The analysis is based on the high-speed synchronous UBVRI photometry of the system after about 56-58 days from the beginning of the outburst's decay. Possible explanations of some features of the light behavior of WZ Sagittae caused by the magnetized white dwarf component is discussed.