COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 445 Konkoly Observatory Budapest 197U July 8 TIME OF MINIMUM FOR WY HYDRAE The eclipsing binary WY Hya was observed photoelectrically on the UBV system on one night in March, 1970 at the No. 1 1.6-inch telescope of the Cerro Tololo Inter-American Observatory. The are just enough observations to roughly determine a time of secondary minimum. Solovyev's /1958/ star "a" was used for, the primary comparison star. Column 1 in Table A lists the heliocentric Julian date. Columns 2, 3 and 4 list the differential V, /B-V/ and /U-B/ magnitude and color indices in the sense variable minus comparison. Table A HJD Delta V Delta /B-V/ Delta /U-B/ 2440676.5689 +1.262 +0.336 -0.126 .5713 1.317 .326 -0.112 .5758 1.409 .292 -0.082 .5780 1.399 .338 -0.102 .5849 1.526 .329 -0.048 .5868 1.532 .331 -0.143 .6006 1.396 .308 -0.130 .6030 1.284 .368 -0.112 .6080 +1.205 +0.334 -0.078 The derived heliocentric Julian Day time of secondary minimum is HJD 2440676.587 +-0.0001. Based upon the ephemeris quoted by Koch, Sobieski and Wood /1963/, the O-C for this secondary minimum is -0.d029 This work was supported by the National Science Foundation. References Koch, R.H., Sobieski, S., and Wood, F.B. 1963,Publ. of Univ. of Pennsylvania, Astronomical Series, Vol.9. Solovyev, A.V. 1958, Peremennye Zvezdy, 12, 626. ARLO U. LANDOLT Louisiana State University Observatory Balton Rouge, Lousiana