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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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Brightness variations of dwarf nova SS Cyg in active states are studied using observations of different outbursts of the system in 2006-2008. The power spectrum analysis of the data reveals the presence of quasi-periodic oscillations in the light curves of SS Cyg near the maximum brightness and at the declinig part of the outburst light curves.