COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 650 Konkoly Observatory Budapest 1972 March 31 INTERMEDIATE-BAND AND H-BETA PHOTOMETRY OF SHORT-PERIOD VARIABLE STARS On seven nights in August, 1969, observations were made at Cerro Tololo Inter-American Observatory in Chile on the following 13 stars, all of which are either known short-period variables or are suspected of short-period variability. The ubvy filters were of the standard type for use in Stromgren intermediate - band photometry. The H-beta filters differed somewhat from those used by Crawford, but the H-beta index has been standardized to that given by Crawford et al. As comparison objects, a number of standard stars were chosen from the lists of D.L. Crawford and J.V. Barnes and from the catalogue of B. Stromgren and C. Perry. In the following table, n refers to the number of separate occasions on which each star was observed. For stars with appreciable amplitudes, the data refer to the mean of the light curve. Star b-y m_1 c_1 beta n HR 242 rho Phe 0.222 0.208 0.771 2.730 4 HR 431 0.210 0.151 0.773 2.713 4 HR 515 0.176 0.167 0.966 2.776 6 HR 5005 0.202 0.165 0.803 2.718 6 HR 6581 omicron Ser 0.055 0.174 1.090 2.891 4 HR 7020 delta Sct 0.207 0.206 0.831 2.714 4 HR 7340 rho Sgr 0.128 0.196 0.962 2.860 4 HR 7928 delta Del 0.195 0.163 0.835 2.758 4 HR 8006 0.180 0.174 0.811 2.781 4 BS Aqr 0.220 0.148 0.834 2.732 10 HD 9133 0.151 0.182 0.940 2.793 4 HD 116994 0.184 0.152 0.863 2.768 10 HD 199757 0.155 0.169 0.860 2.778 10 CARLSON R. CHAMBLISS Department of Physical Sciences Kutztown State College Kutztown, Pennsylvania