The initial mass functions (IMF) of 15 selected open clusters are investigated by making use of C-M diagrams and theoretical evolutionary tracks. Among 15 clusters 13 have peaks in their IMFs and it is thought to be not due to incomplete photometry but to intrinsic property. The mass where IMF peaks is about $2;M_{odot}$ and it is similar to that of the second peak in the IMF of nearby field stars. The mean slope of the IMF in the high mass part is $1.9{pm}0.6$ with some variations among clusters. But there seems to be no correlation between the slope and physical parameters such as ages, diameters, and metal abundances.
