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Analysis of the light curve of the eclipsing close binary system HD 149779.

D. Vander Linden, W. Van Hamme, Maria Jerzykiewicz, Chris Sterken

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Abstract

Observations uvby de cette etoile B 2 IV. Sa variabilite est due aux eclipses. Analyse de ses courbes de lumiere, a l'aide du modele de Wilson Devinney. Les deux composants sont quasi identiques

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What this paper is about

Observations uvby de cette etoile B 2 IV. Sa variabilite est due aux eclipses. Analyse de ses courbes de lumiere, a l'aide du modele de Wilson Devinney. Les deux composants sont quasi identiques

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Available abstract

Observations uvby de cette etoile B 2 IV. Sa variabilite est due aux eclipses. Analyse de ses courbes de lumiere, a l'aide du modele de Wilson Devinney. Les deux composants sont quasi identiques

Key concepts: Physics, Light curve, Astrophysics, Binary star, Binary number, Astronomy, Stars, Arithmetic

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Analysis of the light curve of the eclipsing close binary system HD 149779. — Research Paper | ScholarLens