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AbstractQuasi-simultaneous photometric and polarimetric observations of T Tau and RY Tau show that the proper polarization of these stars barises in the visual region in their gaseous emitting envelopes. The polarization of T Tau shows cyclic variations with a period of 5h18. That of RY has two different modes of variation at brightnesses V > 11mand V < 11m; it is possibly connected with the suspected binary nature of this star.doi:10.1017/s0252921100100569 fatcat:f5oletr74ffjliz2vvmn5qbdsm