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Symbiotic Eclipsing Binary Star CI CYG. The Cold Component Variability
Published online by Cambridge University Press: 12 April 2016
Abstract
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It has been shown that the cold component of CI Cyg eclipsing binary system is a variable star. The amplitude of its light variations is close to with the time interval of 40–60 days.This star being the red giant M4 can be attributed as SR type variability. The light variations is caused by its temperature variations.
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- Session 3. Physics of Individual Objects
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- Copyright © Kluwer 1988