COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1863 Konkoly Observatory Budapest 1980 November 12 HU ISSN 0374-0676 PHOTOELECTRIC MINIMA OF DO CASSIOPEIAE The times of minima of eclipsing variable DO Cas were photoelectrically determined with a 48 cm Cassegrain telescope at the Ege University Observatory. The photometer is equipped with an EMI 9781 A photomultiplier tube and the standard Johnson B, V filters. The heliocentric minima are listed in Table I, where (O-C) values of DO Cas were computed with the help of the light elements given by Cester et al. (1977). Min I = JD Hel. 2433926.4573 + 0.6846661d.E. Table I JD Hel. E (O-C) Filter 2444485.37800 15422 0.00011 B .37855 15422 0.00066 V 498.38564 15441 -0.00091 B .38584 15441 -0.00071 V The photoelectric times of the minima which have been obtained so far by other observers are also shown in Figure 1.The (O-C) values were computed again from the above given equation and plotted against cycles. If the observations obtained in the recent years are examined one can easily assume that DO Cas exhibits decreasing period, since some (O-C) values obtained by other researchers do not fit to the above given equation. But the latest observations of this star, presented in this paper clearly indicate that (O-C) values fit very well to the equation given by Cester et al.(1977). [FIGURE 1] Figure 1. Dots and circles indicate the observations from other researchers and observations obtained at Ege University Observatory, respectively. O. TUMER and S.EVREN Ege University Observatory Bornova-Izmir Turkey Reference: Cester, B., Giuricin, G., Mardirossian, F., and Pucillo, M., 1977, Astron. Astrophys. Suppl. 30, 223 [BIBCODE 1977A&AS...30..223C ]