The a-C : H films have been grown on the glass substrate by PECVD method, where plasma was generated with a 60 Hz line power source. The growth rate of films is found to be dependent of the partial pressure of $C_2H_2$. This growth rate is a little higher than that in which $CH_4$ instead of $C_2H_2$ is used. The transmittance is also much higher(95%). The optical energy gap of films is in the range of 1.4~1.8eV depending on the partial pressure of $C_2H_2$. However, this energy gap, which is 1.8eV, is found to be independent of the partial pressure of $C_2H_2$ for the thick films above $2000{AA}$. The carbonization is checked from peak intensities of D ($sp^3$) and G($sp^2$) peaks in Roman spectra. The hydronization and C-H bonding status in films can also be determined from FTIR results. Both the bonding strength of C-H and the ratio of $sp^3$ to $sp^2$ in bonding are found to be slightly dependent of partial pressure of $C_2H_2$. Judging from above results, we can conclude that the best value for partial pressure of $C_2H_2$ in growing process of thick films is about 13.8%.