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 / Russo, G.; Milano, L.; Maceroni, and C.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - 109:(1982), pp. 368-370.
The Ellipsoidal Binary V 470 Cygni
G. Russo
Membro del Collaboration Group
;L. MilanoMembro 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.File in questo prodotto:
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