Abstract
We report detection of about 30 candidates for pulsating components of eclipsing binaries as a result of the search among over 11,000 eclipsing systems already found in the OGLE-II database of variable star candidates located in Galactic fields. In particular, we found about 15 candidates for δ Scuti stars in Algol-type systems (oscillating EA stars). We found also periodic variations unrelated to the orbital period in the other eclipsing systems. They are likely due to pulsations of one of the components which, depending on the period, can be attributed to δ Scuti,β Cephei or SPB-type variability.
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