  Long-term BVRI photometric light curves of the pre-main sequence stars V977
Cep and V982 Cep during the period from 2000 October to 2016 August are
presented. The stars are located in the vicinity of the reflection nebula NGC
7129. Our photometric data show that both stars exhibit strong photometric
variability in all optical passbands, which is typical for Classical T Tauri
stars. Using our observational data we analyze the reasons for the observed
brightness variations. In the case of V977 Cep we identify previously unknown
periodicity in its light curve.
