Abstract
A Laplace and a Hankel transform of the light curves of eclipsing binary star systems have been expressed in terms of the eclipse elements (L 1,r 1,2 andi) of the spherical basic model. These general expressions can be used for the solution of the eclipse elements of the systems in terms of the observed quantities.
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Demircan, O. Fourier techniques for an analysis of eclipsing binary light curves, VII. Astrophys Space Sci 72, 287–291 (1980). https://doi.org/10.1007/BF00639138
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DOI: https://doi.org/10.1007/BF00639138