Abstrakt
New photoelectric measurements of the eclipsing binary LP Cephei are presented. Period changes could be explain by a light-time effect caused by a third body in an eccentric orbit with a period of 22.5 years.
New photoelectric measurements of the eclipsing binary LP Cephei are presented. Period changes could be explain by a light-time effect caused by a third body in an eccentric orbit with a period of 22.5 years.