COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2309 Konkoly Observatory Budapest 8 April 1983 HU ISSN 0374 - 0676 1981-82 LIGHT CURVE OF II PEGASI A recent note by Byrne et al. (1983) prompts us to make available our 1981 photometry of the interesting RS CVn binary II Pegasi. II Peg was observed differentially on 19 nights between September 1981 and August 1982 with the 48-inch Newtonian at Cloudcroft Observatory. The comparison star was BD + 28d4648, which is C-2 of Byrne et al. The nightly means (which include from 1 to 10 individual differential magnitudes in V of the UBV system) are listed in Table I. Nightly means are plotted in the Figure, where phase is computed with the ephemeris JD 2443030.24 + 6.724183d E. Table I Differential V photometry of II Pegasi in 1981-82 ------------------------------------ JD(hel.) DeltaV JD(hel.) DeltaV 2444000+ 2445000+ ------------------------------------ 872.722 -1.803 120.929 -1.834 873.746 -1.927 121.955 -1.941 874.693 -2.016 153.935 -1.770 893.700 -1.955 158.911 -1.831 956.646 -1.931 160.939 -1.820 966.609 -1.869 167.915 -1.840 967.667 -1.932 168.925 -1.947 977.600 -1.818 187.764 -1.825 188.930 -1.940 191.925 -1.888 196.854 -1.953 ------------------------------------ [FIGURE 1] The first entry in Table I appeared discordant and is not plotted, although the discrepancy might be a result of the light curve's rapid variability rather than measurement error, since these observations span an interval of almost one full year. GREGORY W. HENRY ^a Cloudcroft Observatory Cloudcroft, New Mexico 88317 Reference: Byrne, P. B., Butler, C. J., Andrews, A. D., Rodono, M., Catalano, S., Pazzani, V., Linsky, J. L., Bornman, P., and Haisch, B. M. 1983, I.B.V.S. No. 2258. a) Now at McDonald Observatory, Fort Davis, Texas