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We present new photometric observations of eclipsing binary systems V1241 Tauand GQ Dra. We use the following methodology: Initially, WD code is applied tothe light curves, in order to determine the photometric elements of thesystems. Then the residuals are analysed using Fourier Transformationtechniques. The results show that one frequency can be barely attributed to theresidual light variation of V1241 Tau, while there is no evidence of pulsationon the light curve of GQ Dra.

Asteroseismic Investigation of two Algol-type systems V1241 Tau and GQ Dra