A photometric study of the eclipsing binary V 1073 CYGNI

Details A photometric study of the eclipsing binary V 1073 CYGNI A photometric study of the eclipsing binary V 1073 CYGNI

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.208...15s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 208, no. 1, p. 15-31

Astronomy and Astrophysics

Astrophysics

9

Cygnus Constellation, Eclipsing Binary Stars, Light Curve, Visual Photometry, Atmospheric Correction, Orbital Elements, Stellar Mass

Scientific paper

Photoelectric observations of the eclipsing binary V 1073 Cyg have been
carried out in B and V colors at the Ege University Observatory. The
light curves were analyzed with the Wilson-Devinney approach. A period
study reveals that the orbital period of the system is decreasing at the
rate of (3.21 +/- 0.17) second per century.

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