Multicolor photometry of SU UMa and U Gem during quiescence, outburst and superoutburst

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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4 pages, 2 figures, contribution to the conference proceedings: Interacting binaries: Accretion and Synchronization, 2008, Jun

Scientific paper

The results of time-resolved observations of SU UMa and U Gem obtained over
two-years are presented. Both stars are prototypes of different classes of
dwarf novae. We studied brightness variations on different time scales:
orbital, QPO and flickering. The multicolor BVRI photometry allows to
distinguisch the geometrical and physical sources of these variations.

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