The BVJK Lightcurves of the Shortperiod Eclipsing Binary Cg-Cygni
BVJK light curves of CG Cygni show an apparent infrared excess 0.2 mag out of eclipse, assuming the spectral types of the components to be G9.5V + K3V. The depths of the eclipses also show an excess equal (within the errors) to that at quadrature. The source of these excesses is most probably a circum-system shell of cool material; it cannot be
Bedford, D. K. et al.
Fecha de publicación:
8
1987