COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3160 Konkoly Observatory Budapest 18 March 1988 HU ISSN 0374-0676 THE DISCOVERY OF A BETA LYRAE VARIABLE IN THE VISUAL BINARY SYSTEM ADS 14977 In 1948, Hopmann (1948) listed ADS 14977 (SAO 107139=BD+13d4708) as a suspected variable. Its variability was confirmed this fall at the Flagstaff Station with 650 UBV observations obtained with the 1-m Ritchey-Chretien reflector. The appearance of the light curve, the amplitude and frequency of the light variation, the spectral type (A2) indicate that the A component of ADS 14977 is an eclipsing binary of the Beta Lyrae type. Two primary minima were observed at: T(1)= 244 6731.6339 T(2)= 244 7064.6953, which produced the following light elements: T = 244 6730.18247 + 0.7272018d E The V observations are plotted in Figure 1. The magnitudes and colours of the system, as a function of phase, are given in Table I, These data include the light of the B component (sep.=3.5 arc seconds). Table II lists the magnitudes and colors of the comparison and check stars. Table I Magnitudes and Colors of ADS 14977 Aa x B Phase V B-V U-B 0.00 7.24 0.16 0.04 0.50 7.12 0.12 0.03 0.75 7.05 0.12 0.04 Table II Magnitudes and Colors of the Comparison and Check Stars Star V B-V U-B Comp. SAO 107132=BD+13 4705 8.65 0.53 -0.04 Check SAO 107134=BD+13 4706 9.68 1.13 0.96 The UBV data and light curve analysis (SIMPLEX) are being prepared for publication. Photoelectric CCD observations have been obtained and are being used to remove the light of the B component in the analysis. [FIGURE 1] R.L. WALKER Flagstaff Station U.S. Naval Observatory Flagstaff, AZ 86002 U.S.A. Reference: Hopmann, J.: 1948, Z. Astrophysics, 24, 263. [BIBCODE 1948ZA.....24..263H ]