The triple system CG Aurigae

Several new precise times of eclipses were measured for eclipsing binary CG Aur as a part of our long-term observational project for studying eclipsing binaries with an eccentric orbit. Based on a current O − C diagram, we found for the first time that its orbit is slightly eccentric ( e = 0.124) an...

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Veröffentlicht in:	New astronomy 2011-10, Vol.16 (6), p.402-404
Hauptverfasser:	Wolf, M., Lehký, M., Šmelcer, L., Kučáková, H., Kocián, R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Stars: binaries: eclipsing Stars: fundamental parameters Stars: individual: CG Aur
Online-Zugang:	Volltext
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