We present the results of UBrH(alpha)z monitoring of a sample of T Tau
ri stars. The method of differential CCD photometry was applied. The o
bservations span a range of ten days and show that eleven out of twelv
e sources Varied during this time interval. These variations are corre
lated in all bands. Periods were detected (confidence level 99.99%) fo
r eight out of eleven variable stars; one additional period was found
at the 99.9% confidence level. Of those, one (BP Tau) agrees with prev
iously published periods; two, GM Aur and IQ Tau, do not; six are new
detections of periodicities. The sample is drawn from the Taurus-Aurig
a and Cepheus IV star-forming regions.