RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Keywords

Eclipsing Binaries:Light Curves
Eclipsing Binaries:Photometry
Light Curves:Eclipsing Binaries
Photometry:Eclipsing Binaries
W UMa Stars

How to Cite

Observaciones fotoelectricas UBV y analisis de binarias eclipsantes de corto período: AU Phoenicis, SY Horologii y VY Ceti. (1985). Revista Mexicana De Astronomía Y Astrofísica, 10(1), 283-291. https://astronomia.unam.mx/journals/rmxaa/article/view/1985rmxaa..10..283l

Abstract

The first photoelectric observations of three eclipsing binaries (AU Phe, SY Hor and VY Cet) with periods around 0.3 days and spectral types G and K are presented. The light curves of these systems show W UMa-type characteristics with partial eclipses. The Wilson and Devinney model is employed to analyse the light curves in the V-magnitude. Different sets of possible solutions are presented and discussed.
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