COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1642 Konkoly Observatory Budapest 1979 July 17 THE SECONDARY PERIOD OF RZ CEPHEI We have analized the 20 light maxima obtained by Todoran during 1972-1973 (I.B.V.S. No.915, 1974) and 2 maxima observed in the same period by Cester and Todoran (Mem.SAIt, 47, 217). At first we have derived the following elements valid from J.D.2441475 to J.D.2442006: Max.hel = 2441475.378+ 0.30868218d*E (1) Table I contains the 22 maxima and the O-C values derived from the ephemeris (1). Based on an harmonic analysis we have derived the secondary period of the star: P_b = 96.8 P_0 = 29.88d. In Figure 1 the values of O-C are plotted against the phase of the secondary period computed by the formula: Lowest Maximum = 2441464.147+ 29.88d*N (2) The phases of the light maxima performed with the elements (2) are given in third column of Table I. [FIGURE 1] Table I Max. hel. 2440000 O-C psi 1475.380 +0.002d 0.38 1519.519 0.000 0.85 1546.372 -0.003 0.75 1559.339 0.000 0.19 1605.335 0.002 0.73 1605.640 -0.002 0.74 1608.420 0.000 0.83 1897.350 0.004 0.50 1902.286 0.001 0.66 1902.592 -0.002 0.67 1903.520 0.000 0.70 1904.445 -0.001 0.74 1907.530 -0.003 0.84 1942.410 -0.004 0.01 1946.425 -0.002 0.14 1963.402 -0.002 0.71 1975.439 -0.004 0.11 1984.396 0.001 0.41 1985.325 0.004 0.44 1991.190 0.004 0.64 1991.495 0.001 0.65 2006.310 -0.001 0.14 FEDERICO FICARROTTA CLAUDIO ROMOLI Observatory of Monte Zufolone Technical Direction Via Garibaldi 3 I-20013 Magenta (Milano) Italy