COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2791 Konkoly Observatory Budapest 13 September 1985 HU ISSN 0374 - 0676 LIGHT CURVE VARIATION OF PZ CASSIOPEIAE The semi-regular variable star PZ Cassiopeiae was investigated using the patrol plates of Odessa astronomical observatory seven-camera astrograph obtained in 1957-1983. They were exposed through a yellow filter on the emulsion ZP-3. The exposure time was 30 min. The times of light extrema observed are given in Table I. For them the following elements were obtained (L.S. Kudashkina, Astron.Tsirk. No. 1351, 1984): Max JD = 2436809.6 + 801.3d E Min JD = 2437164.1 + 801.3d E The diagram for residuals (O-C) for the above elements is shown in Figure 1. Maximum and the subsequent minimum have the same cycle number. Qualitative similarity of (O-C) curves for maximum and minimum shows that cycle duration is changing, possible in a regular way. The dependence of duration of the ascending and descending branches on cycle number (which corresponds to the nearest maximum) is shown in Figure 2. As these two curves are opposite in phase, cyclicity (about 18 years) cannot be excluded. Ascending branch is shorter than the descending one during half of this cycle but in the second half of the cycle the situation is inverse. Table I E Max O-C Min O-C 0 2436900 91 2437180 16 1 7600 -10 7940 -25 2 8320 -22 8700 -67 3 9000 -214 9610: 42 4 9840 -175 2440520 151 5 2440800 -16 1220 49 6 1600 -17 1980 8 7 2680: 162 2800 27 8 3400 180 3600: 26 9 4120 99 4360: -16 10 4800 -23 5260: 83 11 5660 36 Author is grateful to Yu.S. Romanov and I.L. Andronov for useful discussions. [FIGURE 1] [FIGURE 2] L.S. KUDASHKINA Odessa State University T.G. Shevchenko Park Odessa 270014 USSR