COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1337 Konkoly Observatory Budapest 1977 September 9 NEW PHOTOELECTRIC OBSERVATIONS OF THE DELTA SCUTI STAR HD 73576 (KW 207) The delta Scuti star HD 73576 (KW 207), belonging to the Praesepe cluster, was observed during one night only by M. Breger (Astrophys.J. 162, 597, 1970). The same author (Astrophys. J. 176, 373, 1972) assigns it a tentative period of 0.071d. We have performed photoelectric observations of this star through B filter during four nights at the beginning of 1977, using the 102-cm reflector of the Merate Observatory. The comparison star, whose constancy we have verified, was HD 73619 (KW 229): it does not vary to an extent of greater than 0.003m. The resulting light curves (mc-mv) for the first three nights (J.D. 43168, ...173 and ...174) are shown in Fig. 1, whereas Fig. 2 shows the curve relative to the last night (J.D.43203). The observed trend of Fig. 1 is not significantly different from a simple sinusoid. This fact is confirmed by a spectral analysis with Vanicek's method (Astrophys.Space Sci. 12, 10, 1971), which also gives, for the period, the value of 0.0534d. It is apparent in the last night the situation is at all different. The analysis gives a non-monochromatic periodogram, with the main peak at 0.059d. Another, much less marked peak corresponds to a period of 0.068d, and there is perhaps another one at about 0.051d. The 0.0534d component seems to be disappeared. Anyway there is no evidence for the Breger's period. It is our intention to continue with the observations. M. BOSSI G. GUERRERO L. MANTEGAZZA Osservatorio Astronomico Via E. Bianchi 46 22035 Merate (Como), Italy [FIGURE 1] [FIGURE 2]