Hostname: page-component-745bb68f8f-lrblm Total loading time: 0 Render date: 2025-01-11T06:01:46.155Z Has data issue: false hasContentIssue false
  • English
  • Français

Symbiotic Eclipsing Binary Star CI CYG. The Cold Component Variability

Published online by Cambridge University Press:  12 April 2016

T.S. Belyakina
T.S. Belyakina*
Affiliation:
Crimean Astrophysical Observatory 334413, Nauchny, Crimea, USSR

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Session 3. Physics of Individual Objects
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 197
Copyright
Copyright © Kluwer 1988