COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1078 Konkoly Observatory Budapest 1975 December 28 PHOTOELECTRIC OBSERVATIONS OF VZ Cnc (HD 73857) The observations were made during four nights in 1967/68 by Klement and Sterzinger with the 24" refractor of the University Observatory in Vienna. Measurements in the blue and yellow spectral region were obtained around maximum light. In 1974, UBV- observations over two cycles were obtained during two nights by Hahn and Lustig with the 60 cm photometric reflector of the Observatoire de Haute Provence (OHP). From the light-curves we determined the maxima and the moment of occurrence of the median magnitude on the ascending branch T (m),m = 0.5 (m_max + m_min). The reduction of the data brought no changes of either the primary or the beat period. It would be necessary to get long runs over two or three primary cycles to be able to detect a possible variation of the beat period (P_p= 0.17836376d, P_b= 0.716292d, ref. W.S. Fitch, Ap.J. 121, 690, 1955). The observational data are summarized in the following table. -------------------------------------------------------------- Date of T_max T(m) Amplitude Observers Observations JD hel JD hel -------------------------------------------------------------- 1967.12.28/29 243 9852.6396d 243 9852.6347d 0.67m Klement, Sterzinger 1968.01.22/23 9878.5006 9878.4962 0.55 Klement, Sterzinger 1968.01.23/29 9879.3958 9879.3896 0.43 Klement, Sterzinger 1968.02.16/17 9903.4730 Klement, Sterzinger 1974.02.20/21 244 2099.5045 244 2099.4851 0.67 Hahn,Lustig 1979.02.21/22 2100.3915 0.49 Hahn,Lustig -------------------------------------------------------------- GERHARD HAHN HANS JASICEK GUNTER LUSTIG GERHARD KLEMENT University Observatory University Observatory A-8010 Graz, Austria (Amateur-Group) A-1180 Vienna, Austria