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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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Here we report the results of CCD observations which were carried out during the outbursts of dwarf novae V1251 Cyg, KP Cas and UW Tri. All observations were made in October-November 2008 with 60-cm and 38-cm telescopes in Crimea. Our data clearly show the presence of superhumps in the light curves of these systems. The evolution of superhumps was followed up. The amplitudes and periods of detected modulations were estimated from the hump maxima. A comparison with the previous outbursts is also provided.