Long-term starspot activity of CG Cygni.

Physics

Scientific paper

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Rs Cvn Stars: Starspots, Rs Cvn Stars: Stellar Activity

Scientific paper

CG Cygni is a member of the short-period group of RS CVn stars. It is
found that one large active region at high latitude (≍45°) in
one active longitude belt (≍90° or 270°) usually explains
the distortion waves in the photometric data.

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