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The BVRcIc CCD photometry in the fields of six open clusters toward thePerseus spiral arm is presented. These data along with JHKs magnitudes takenfrom 2MASS catalog, have been used to determine cluster's ages, distances andcolor excesses. In addition, the gaps in mass function of Be 97, King 12 andNGC 7788 clusters have been revealed in mass intervals of 1.3-1.5, 1.4-1.6 and1.5-1.7 solar masses, respectively.

Photometric study of open clusters Berkeley 96, Berkeley 97, King 12, NGC 7261, NGC 7296, and NGC 7788