Abstract:We present the results of high-resolution (0.24Å/pix) monitoring of the variability of Hα and He I 6678 lines in the spectrum of X Per in 1996-99 at Tartu Observatory. The main characteristics of the line variability distinguishable in our data are:1) the intensity of emission peaks in both lines varies with a cycle-length ≈450 days, and displays a phase-lag between curves of two lines considered,2) in a cycle, both violet or red emission peaks emerge at high Doppler velocities but attain their maxima and disa… Show more
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