S. A. Naftilan scite author profile

A new CCD light curve of the A-type W UMa star V1073 Cygni has been obtained, and the di †erential-corrections method of Wilson and Devinney was used to compute a new set of system parameters. The same analysis has been applied to the other photometric light curves in the literature, including the Hipparcos light curve. A new ephemeris is determined for the times of primary minimum. V1073 Cygni probably has initially formed as a detached system and evolved into contact.

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A spectroscopic study of the close binary CG Cygni

Naftilan¹,

Milone²

1979

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S. A. Naftilan

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Recent photometry of CG Cygni

V1073 Cygni: A New Light Curve and Analysis

A spectroscopic study of the close binary CG Cygni

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