Photometric Analysis of the Eclipsing Binary V1425 Cygni

Details Photometric Analysis of the Eclipsing Binary V1425 Cygni Photometric Analysis of the Eclipsing Binary V1425 Cygni

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.241..327d&link_type=abstract

Astrophysics and Space Science, Volume 241, Issue 2, pp.327-332

Astronomy and Astrophysics

Astrophysics

Scientific paper

Photoelectric B and V light curves of the eclipsing binary V1425 Cygni
were analyzed by the method of Wilson-Devinney. The system was found to
be a semi-detached binary where the secondary component (less massive
and cooler) fills its Roche lobe.

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