COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1273 Konkoly Observatory Budapest 1977 May 5 TWO DELTA SCUTI STARS IN THE PLEIADES Observations of two Delta Scuti suspects in the Pleiades cluster were obtained using the 40-cm reflector and a dry ice cooled 1P21 at the Grundy Observatory. An OG-4 (4mm) filter approximates the V magnitude. Observations were made differentially between variable and comparison, and extinction was removed. Light curves were analyzed using a periodogram technique after Gray and Desikachary (1973, Ap. J. 181, 523). Stars are identified by TR numbers (Trumpler 1921, Lick Obs. Bull. 10, 110). Breger (1972, Ap. J. 176, 367) reported TR 51 a possible Delta Scuti star with a period of about 0.024+-0.002 days and an amplitude of about 0.01 magnitudes. TR 51 was observed on one night with TR 121 as a comparison star. Periodogram analysis of the data gives a period of 0.0205 days with an amplitude of 0.01 magnitudes peak to peak. Subtraction of this peak and its side lobes reveals a second maximum at a period of 0.017 days with an amplitude of about 0.007 magnitudes peak to peak. Breger also reported TR 390 as a possible Delta Scuti star with a period of 0.049+-0.004 days and an amplitude of 0.01 magnitudes. Observations of TR 390 were obtained on one night using TR 365 as a comparison star. Periodogram analysis of the data reveals a period of 0.047 days and an amplitude of 0.011 magnitudes peak to peak, in good agreement with Breger. Removal of this variation from the periodogram reveals a second peak at 0.070 days with a peak to peak amplitude of about 0.006 magnitudes. Beat phenomenon is likely in both TR 51 and TR 390. Further observations are needed to confirm periods and amplitudes. Joseph R. Grundy Observatory MICHAEL A. SEEDS Franklin & Marshall College Lancaster, PA. 17604, U.S.A. CHARLES J. STEPHENS