The preliminary results of the eclipsing binary system EW Boo with a δ Scuti component

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Scientific paper

We present the first ground-based photometric observations and results
of EW Boo. The V light curve obtained over 12 nights in 2006 was
analyzed by using the Wilson-Dewinney code. We also found that the
primary component of the system shows δ Scuti-type variability.

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