SIMBAD references

Spectroscopic observations around the H_α line and BVR photometry of the eclipsing short-period RS CVn-star CG Cyg are presented. The solutions of the radial velocity curves and the light curves yielded the following masses and radii of the star components: M₁=0.97M_☉, M₂=0.80M_☉, R₁=1.00R_☉, R₂=0.83R_☉. The measured rotational broadenings of the observed lines correspond to equatorial velocities V₁=80km/s and V₂=66km/s. The distortions of our multicolor light curve were reproduced by two cool spots on the primary star. The strong absorption feature between the spectral lines of the two stars was explained by extended structure around the mass center of the system. The H_α emission line of the secondary star in the August spectra was attributed to a prolonged flare of this star.