V1073 Cygni: A New Light Curve and Analysis

Details V1073 Cygni: A New Light Curve and Analysis V1073 Cygni: A New Light Curve and Analysis

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000pasp..112..852m&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 112, Issue 772, pp. 852-860.

Astronomy and Astrophysics

Astronomy

4

Stars: Binaries: Close, Stars: Binaries: Eclipsing, Stars: Individual: Constellation Name: V1073 Cygni

Scientific paper

A new CCD light curve of the A-type W UMa star V1073 Cygni has been obtained, and the differential-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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