The yellow and blue photoelectric lightcurves -as yet unsolved- of the double lined spectrum binary V470 Cyg (Ebbighausen et al. 1975) have been analyzed by means of the Wilson and Devinney (1971) method. The systeffi turns out to be a detached one, with two almost equal B2-B3 components, which do not eclipse each other because of che very low inclination (~50°). At primary minimum, the bigger and more massive star is in front.

The Ellipsoidal Binary V 470 Cygni

G. Russo
Membro del Collaboration Group
;
L. Milano
Membro del Collaboration Group
;
1982

Abstract

The yellow and blue photoelectric lightcurves -as yet unsolved- of the double lined spectrum binary V470 Cyg (Ebbighausen et al. 1975) have been analyzed by means of the Wilson and Devinney (1971) method. The systeffi turns out to be a detached one, with two almost equal B2-B3 components, which do not eclipse each other because of che very low inclination (~50°). At primary minimum, the bigger and more massive star is in front.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11588/892634
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