Photometry and analysis of the eclipsing binary V909 Cygni

Details Photometry and analysis of the eclipsing binary V909 Cygni Photometry and analysis of the eclipsing binary V909 Cygni

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...73..255g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 73, no. 2, May 1988, p. 255-263.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Light Curve, Spectrum Analysis, Stellar Spectrophotometry, Astronomical Catalogs, Electrophotometry

Scientific paper

The first photoelectric observations of the photometrically neglected eclipsing binary V909 Cygni in blue and yellow colours are presented. It was found that the orbital period of the system should be twice that of given in the catalogues. The light curves were analysed by means of Wood's model simulation program WINK. The system was found to be a detached binary.

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