COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1938 Konkoly Observatory Budapest 1981 March 17 HU ISSN 0374-0676 TIMES OF MINIMA OF TEN ALGOL-LIKE BINARIES We give times of minima for 27 primary eclipses of 10 Algol-like binaries. Most observations were made with the 1.0 M Prairie Observatory reflector, with single-channel pulse-counting photometer, RCA C31034A-02 photomultiplier, and Stromgren-Crawford uvby and Kron I filters. Two minima were also obtained using the 0.4 M Mt. Laguna reflector with single-channel PC integrator photometer, RCA 1P21 photomultiplier, and uvby filters. Times of minima for each color were determined in most cases by the method of Kwee and Van Woerden (1956) and programmed by R.C. Crawford. TABLE I TIMES OF PRIMARY MINIMA SHOWING NO WAVELENGTH DEPENDENCE Binary HJD- Binary HJD- 2440000 2440000 XZ And 3779.8763 +- 0.0001 ST Per 3821.6554 +- 0.0002 3809.7364 +- 0.0001 3882.5664 +- 0.0001 3847.7403 +- 0.0001 4120.9133 +- 0.0002 4257.6387 +- 0.0001 4520.8075 +- 0.0007^c 4542.6659 +- 0.0000 U Sge 4374.8182^a KO Aql 3737.655 +- 0.001^a 4049.836 +- 0.001^a RW Tau 3820.7835 +- 0.0001 4387.7954 +- 0.0001^b 4180.7319 +- 0.0001 W Del 4438.7465 +- 0.0001 X Tri 3760.8573 +- 0.0000 4462.7765 +- 0.0002 3831.7795 +- 0.0002 4171.8186 +- 0.0001 4546.8309 +- 0.0001 a: Graphical determination. b: Correction to I.B.V.S. No. 1840. c: y, b, v only; I, u eclipses were asymmetrical or noisy. TABLE II TIMES OF PRIMARY MINIMA SHOWING WAVELENGTH DEPENDENCE HJD - 2440000 Binary I y b v u SW Cyg 4428.7625 .7631 .7634 .7640 .7647 +-.0003 +-.0001 +-.0001 +-.0001 +-.0003 ----- 4460.7738 .7745 .7754 .7762 +-.0007 +-.0008 +-.0004 +-.0004 RW Mon^a 3883.7712 .7708 .7708 .7709 .7714 +-.0001 +-.0001 +-.0001 +-.0001 +-.0001 RV Oph 4427.7251 .7251 .7251 .7254 .7255 +-.0002 +-.0001 +-.0001 +-.0002 +-.0002 RW Tau 4191.8080 .8076 .8074 .8072 .8085 +-.0001 +-.0001 +-.0001 +-.0001 +-.0001 4587.7519 .7515 .7513 .7511 .7523 +-.0001 +-.0002 +-.0000 +-.0000 +-.0001 a: Replaces the single time given in I.B.V.S. No.1840. Table I lists times and mean errors for binaries in which times were wavelength-independent. Table II tabulates those times showing wavelength dependence. Apparent time of mid-eclipse is always latest in the ultraviolet. McNamara and Feltz (1976) noted in U Sge that ultraviolet times were delayed from yellow, blue, and violet times by ~ 43 seconds, and Crawford (1979) remarked on ultraviolet delays in U Cep as large as 11 minutes. Among the systems of Table II, earliest times range from infrared in SW Cyg to violet in RW Tau. The maximum time spread is from 35+-19 sec (RV Oph) to 190+-37 sec (SW Cyg). All of these systems apparently are affected by circumstellar effects of mass transfer, as discussed by Crawford (1979) and Olson (1980). The author thanks the National Science Foundation for support of this work, and Dr. Burt Nelson for observing time and assistance at the Mt. Laguna Observatory. Mr. Dean Espitallier and Mr. Tom Bryant assisted with observations of SW Cyg and W Del at Mt. Laguna Observatory. EDWARD C. OLSON Astronomy Department University of Illinois at Urbana-Champaign 1011 W. Springfield Urbana, IL 61801, USA References: Crawford, R.C. 1979, Publ. A.S.P., 91, 111. [BIBCODE 1979PASP...91..111C ] Kwee, K.K., and Van Woerden, H. 1956, Bull. Astr. Inst. Netherlands, 12, 327. [BIBCODE 1956BAN....12..327K ] McNamara, D.H., and Feltz, K.A. 1976, Publ. A.S.P., 88, 688. [BIBCODE 1976PASP...88..688M ] Olson, E.C. 1980, I.B.V.S. No. 1839.