Abstract
We found for the first time that orbit of CG Aur is slightly eccentric and that times of minima besides the slow apsidal motion show very rapid changes, caused probably by the third body orbiting the eclipsing pair.
We found for the first time that orbit of CG Aur is slightly eccentric and that times of minima besides the slow apsidal motion show very rapid changes, caused probably by the third body orbiting the eclipsing pair.