COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 1478 Konkoly Observatory Budapest 1978 September 27 PHOTOELECTRIC MINIMA OF SEVEN ECLIPSING BINARIES AND A SINGLE MAXIMUM OF BW VULPECULAE We report herein photoelectric observations of seven eclipsing binaries and BW Vulpeculae made in 1975 and 1976 with the 40-cm Boller and Chivens f/18 Cassegrain telescope of the University of Montana. This telescope, located on 1980-meter Blue Mountain about six air miles southwest of the university campus, is equipped with an Astro Mechanics single-channel photometer containing an unrefrigerated EMI 6256B PM tube. The observations were made through a Corning 3384 V-band filter. The photomultiplier signal is fed through a DC amplifier to a voltage-to-frequency converter, whose output is integrated for ten seconds by an electronic counter. Three such integrations constitute a single observation. The observations were reduced by computer to produce extinction-corrected differential visual magnitudes (program star-comparison star) as a function of heliocentric Julian Date using the photometry reduction program of Walter Fitch (Steward Observatory). The heliocentric times of the observed minima were determined graphically by the chord bisection method. Table 1 lists the observed times of minimum and their probable errors, the epoch numbers E, and the O-C values. Table 2 gives the ephemerides used to calculate the O-C values. Table 1. Observed Heliocentric Times of Minimum Star Hel. JD - 2440000 E O-C KO Aql 2637.8558 +- 0.0005 262 +0d0085 44i Boo 2619.8345 +- 0.0015 10,333 +0.0025 RZ Cas 2633.7591 +- 0.0002 10,674 -0.0008 2664.8340 +- 0.0001 10,700 -0.0023 2670.8114 +- 0.0003 10,705 -0.0012 3049.7003 +- 0.0008 11,022 -0.0056 TW Cas 2666.8395 +- 0.0014 461 -0.0047 3096.7636 +- 0.0003 762 -0.0073 3103.9140 +- 0.0004 767 +0.0014 DO Cas 2636.7778 +- 0.0003 12,722 +0.0003 2664.8447 +- 0.0003 12,763 -0.0041 XX Cep 2663.7476 +- 0.0003 1866 +0.0062 AT Peg 2661.8070 +- 0.0006 1940 -0.0197 Table 2. Ephemerides for Eclipsing Binaries Star Heliocentric JD Period (days) Source KO Aql 2,441,887.4714 2.86403 SAC 49 44 iBoo 2,439,852.4903 0.2678159 Durbeck RZ Cas 2,429,875.6902 1.1952473 Herczeg and Frieboes-Conde TW Cas 2,442,008.3850 1.428328 SAC 49 DO Cas 2,433,926.4573 0.68466595 SAC 49 XX Cep 2,438,302.3209 2.33731 SAC 49 AT Peg 2,440,438.383 1.146105 SAC 49 Minima of AT Peg observed in 1974 and 1976 by Pohl and Kizilirmak (1974; 1976) also give negative O-C's, based on the ephemeris used here, of -0.0041 and -0.0118, respectively, suggesting a possible decrease in the period of AT Peg of the order of 0d.00001 since 1969. The observed maximum of BW Vul was found to occur at Hel. JD (Max) = 2,443,060.6544 +- 0.0005. The parabolic ephemeris equation derived by Valtier (1976) applied to the above time yields O-C = +0.0156 days, while the linear ephemeris equation of Tunca (1978) yields O-C = -0.0014 days. T.E. MARGRAVE, J.H. DOOLITTLE, D. CUTILLO, and J.S. SCHERRER Blue Mountain Observatory University of Montana Missoula, Montana 59812 USA References : Durbeck, H. W.: IBVS No. 1023, 1975. Herczeg, T. and Frieboes-Conde, H.: Astr. and Ap., 30, 259, 1974. [BIBCODE 1974A&A....30..259H ] Kordylewski, K.: Supplemento ad Annuario Cracoviense No. 49, Krakow 1977. Pohl, E. and Kizilirmak, A.: IBVS No. 937, 1974; IBVS No. 1163, 1976. Tunca, Z.: IBVS No. 1386, 1978. Valtier, J.-C: Astr. and Ap., 51, 465, 1976. [BIBCODE 1976A&A....51..465V ]