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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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The program of CCD photometric monitoring of bright supernovae (SNe) is carried out at 0.4 -1.0 meter telescopes of Sternberg Astronomical Institute, Crimean Astrophysical Observatory and Stara Lesna Observatory since 1998. We have observed more than 250 SNe of different types. We present the results of observations of SNe Ia 2003du, 2009nr and 2011fe, type IIb SNe 2008ax, 2011dh, type II SNe 2004ek and 2005kd and discuss physical parameters of the explosions.