SIMBAD references

We present the results from optical photometric and spectroscopic observations of the pre-main-sequence (PMS) stars V1184 Tau and V350 Cep. Both objects pass through an optical outburst and they were considered as fuor candidates in previous studies. The long-term light curve of V350 Cep resembles fuor-type stars, but its spectrum is similar to classical T Tauri stars. In the period of observations, V1184 Tau remained at the maximum brightness. Significant changes in the profile and strength of emission lines were found.