Abstract
The aim of the present paper has been to generalize the method, developed by Kopal (1976), for the evaluation of the photometric proximity effects (between minima as well as within eclipses) of distorted eclipsing systems. The method is extended to quantities of second order (n-7) is surficial distortion. Analytical expressions of the polynomials to be used for ‘modulation’ of the light curve are also given.
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Niarchos, P.G. On the evaluation of the photometric proximity effects of close eclipsing systems. Astrophys Space Sci 76, 503–511 (1981). https://doi.org/10.1007/BF00687509
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DOI: https://doi.org/10.1007/BF00687509