The Light Curve Variations of The Active Binaries With Hot Subdwarf Component
Esin Sipahi, Serdar Evren
Abstract
We present the light curve variations of the two active binaries with hot subdwarf component. According to the brightness variations outside of the eclipses, the giant components of the systems are chromospherically active stars. The dark and cool active structures on this components cause the variations of the total light of the systems.
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