COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1245 Konkoly Observatory Budapest 1977 February 28 ON THE BLAZHKO EFFECT IN AR Ser As has already been reported (V.P. Tsessevich, AC, No. 885, 1975) AR Ser shows anomalous Blazhko effect. The height of maximum light of this star as well as its time shift (O-C) relative to linear elements vary periodically. I made observations of this star in the interval JD 2442126- JD 2442994. For the Blazhko effect the following formula has been obtained by us: 1) T_max = 2442195.5+ 108.4 x n The shift of the moments of maximum light (O-C) has been determined from the elements: 2) Max.hel. JD = 2442126.441+ 0.575092 E. On the basis of our observations we may conclude that the amplitude of Blazhko effect in AR Ser changes, possibly in cyclic way (see Figures 1, 2, 3). The moments of maximum light, the heights of maximum light, E_2, (O-C)_2 and phases of Blazhko effect, derived from formula (1) are given in Table below: Table Max.hel.JD m_v E_2 (O-C)_2 Psi1 2442126.441 12.09 0 0.000 0.363 134.504 11.99 14 .012 .437 137.383 11.96 19 .015 .464 187.406 11.63 106 .005 .925 198.338 11.55 125 .010 .026 199.489 11.63 127 .011 .037 206.390 11.68 139 .011 .100 214.432 11.78 153 .002 .175 218.464 11.85 160 .008 .212 221.333 11.89 165 .002 .238 225.380 11.91 172 .023 .276 244.342 12.22 205 .007 .451 486.497 12.07 626 .048 .684 490.492 12.02 633 .018 .721 512.390 11.84 671 .062 .923 542.426 12.09 723 .194 .200 546.934: 12.13: 730 .144 .237 576.331 12.16 782 .168 .512 580.360 12.14 789 .172 .550 868.463 12.16 1290 .153 .208 872.474 12.18 1297 .139 .245 918.394 12.18 1377 .051 .669 922.373 12.12 1384 .005 .705 926.401 12.14 1391 .007 .743 934.448 12.05 1405 .003 .817 937.340 12.04 1410 .019 .844 945.372 12.02 1424 .000 .918 949.420 11.87 1431 .022 .955 953.454 12.04 1438 .031 .992 960.355 11.97 1450 .031 .056 979.340 12.15 1483 .038 .231 990.324 12.18 1502 .095 .332 994.349: 12.25: 1509 .094 .369 B.N. FIRMANYUK Odessa Astronomical Observatory [FIGURE 1] [FIGURE 2] [FIGURE 3]