COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2771 Konkoly Observatory Budapest 7 August 1985 HU ISSN 0374 - 0676 THE J LIGHT CURVE OF CG CYGNI We present the J light curve of the eclipsing binary CG Cygni (P=0.63d) obtained with the 1.5 m infrared flux collector at the Observatorio del Teide, Tenerife, using a cooled InSb detector. The data were obtained during 4 out of 5 consecutive nights in September 1984. The comparison star was BD+34deg 4216 and the principal standard star was BS8430. In Figure 1 is the J light curve of CG Cygni with the differential magnitude plotted against the phase, calculated using the ephemeris of Milone and Ziebarth (1974) JD(phase=0) = 2439425.1221 + 0.6311410d E. [FIGURE 1] Figure 1: J light curve of CG Cygni. The J light curve shows the asymmetry of the minima that has been previously observed in optical curves of CG Cygni (Milone et al. 1979; Jassur, 1980) and some other short period RS CVn-type binaries. Figure 1 also shows that the minima have advanced in phase by about 2.5% since 1966, confirming conclusively the progressive change first noted by Milone et al. A fuller account of this work is being prepared for publication. J.J. FUENSALIDA, M. J. AREVALO D. K. BEDFORD Instituto de Astrofisica de Canarias Dept. of Space Research La Laguna University of Birmingham Tenerife, Spain Birmingham, U.K. References : Jassur, D.M.Z.: 1980, Astrophys. Space Sci. 67, 19. [BIBCODE 1980Ap&SS..67...19J ] Milone, E.F., Ziebarth, K.E.: 1974, Pub. Astron. Soc. Pacific 86, 684. [BIBCODE 1974PASP...86..684M ] Milone, E.F., Castle, K.G., Robb, R.M., Swadron, D., Burke, E.W., Hall, D.S., Michlovic, J.E., Zissell, R.E.: 1979, Astron. J. 84, 417. [BIBCODE 1979AJ.....84..417M ]