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Parameters of the Dwarf Nova SS Cygni Obtained From UBV Photoelectric Light Curve Analysis

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Irina Voloshina
Tatiana Khruzina

Sternberg Astronomical Institute, Universitetskij pr.13, Moscow, Russia

We present the results of analysis of UBV-photoelectric mean light curves of SS Cygni at quiescence.

Link to article on ADS

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