Classification of the Fine Effects in the Light Curves of Eclipsing Binary Stars

Details Classification of the Fine Effects in the Light Curves of Eclipsing Binary Stars Classification of the Fine Effects in the Light Curves of Eclipsing Binary Stars

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..35..177k&link_type=abstract

The Journal of the American Association of Variable Star Observers, Vol. 35, No. 1, p. 177

Physics

1

Scientific paper

This paper discusses the fine effects in photoelectric light curves of eclipsing binary stars, and shows the classification of fine effects and their deformational influence on a light curve if they are present in the binary system. More detailed analysis is denoted to one of them-effect of refraction electromagnetic radiation in the atmospheres of close binary stars. This effect deforms the light curve during the total eclipse. On the light curve it is manifested by the small hump in the constant part of the minimum. This effect is registered in seventeen systems.

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