Photoelectric photometry of the eclipsing binary V1425 Cygni

Details Photoelectric photometry of the eclipsing binary V1425 Cygni Photoelectric photometry of the eclipsing binary V1425 Cygni

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..283g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 2, July 1988, p. 283-297. Research supported by Aegean University

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Electrophotometry, Least Squares Method, Stellar Color, Stellar Luminosity, Stellar Magnitude

Scientific paper

Photoelectric differential B and V magnitudes of the eclipsing binary
V1425 Cygni are presented yielding the complete photoelectric light
curve of this relatively bright system. The improved light elements are
calculated using the least-squares method.

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