COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3662 Konkoly Observatory Budapest 20 September 1991 HU ISSN 0374 - 0676 PHOTOELECTRIC MINIMA OF THE ECLIPSING BINARY XY BOOTIS The variability of XY Boo (BD+20d 2874) was discovered by Hoffmeister (1935). It was found by Tsesevich (1950) that the system belonged to the W UMa type. The system was observed photoelectrically at the Yunnan Observatory in yellow and blue colours using a 60 cm reflector telescope and a photoelectric photometer equipped with an EMI 8256B photomultiplier tube and Johnson's standard B, V filters. The integrations were controlled by a microcomputer. Integration of each observation is twenty seconds. The comparison and check stars are the same as that used by Binnendijk (1971). Five minima and the values of E and O-C obtained in both B and V filters for XY Boo are listed as follows: JD.Hel. Min. Filter E O-C 2448334.3320 II V 21439.5 0.1390 .3319 B 0.1389 2448335.2623 I V 21442 0.1433 .2624 B 0.1434 2448336.3700 I V 21445 0.1390 .3704 B 0.1394 2448363.2365 II V 21517.5 0.1404 .2360 B 0.1399 2448364.1655 I V 21520 0.1435 .1660 B 0.1440 The O-C values were calculated using Binnendijk's ephemeris (1971): JD.Hel.Min.I = 2440389.7321 + 0.37055251 E. ZHANG YUNLIN, LIU QINGYAO, WANG BI and GU SHENHONG Yunnan Observatory Academia Sinica Kunming, P.O. Box 110 People's Republic of China References: Binnendijk, L.: 1971, Astron.J. 76, 923. [BIBCODE 1971AJ.....76..923B ] Hoffmeister, C.: 1935, Astron. Nachr. 255, 401. [BIBCODE 1935AN....255..401H ] Tsesevich, V.P.: 1950, Astron. Circ. Kasan (No. 100), 18.