Steven L. Morris 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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Dominant Flow Structures In The Wake of A Cyclist

Crouch¹,

McGrath

Thompson³

et al. 2012

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The Limits of Inclination for Binary Star Partial Eclipses

Morris

1999

ApJ

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Steven L. Morris

The ellipsoidal variable stars

The Equations of Ellipsoidal Star Variability Applied to HR 8427

V1073 Cygni: A New Light Curve and Analysis

Dominant Flow Structures In The Wake of A Cyclist

The Limits of Inclination for Binary Star Partial Eclipses

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