Abstract
The aim of the present paper will be to present a new approach to the light changes of eclipsing binary systems. The light changes have been expanded into the Fourier-Bessel and Dini series. The coefficients of these expansions which are the Hankel transforms of the order μ of the loss of light (1−l) have been expressed in terms of the eclipse elements. These discrete Hankel transformsH μ(j m ) andH μ(λ m ) valid for only the positive real zerosj m andλ m of the functionsJ λ and [xJ′μ(x)+ϱJ μ(x)] have been generalized for any positive value of μ andy. Thus, these general expressions for the Hankel transforms of the light curves which are valid for all types of eclipses, for any arbitrary degree of the adopted limb-darkening law and, moreover, for any positive value of the free parameters μ andy, may be used for the solution of the elements of eclipsing binary systems.
Similar content being viewed by others
References
Abramowitz, and Stegun, I. (eds.): 1964,Handbook of Mathematical Functions with Formulas, Graphs and Mathematical Tables. Appl. Math. Ser. 55, U.S. Govt. Printing Office, Washington, D.C.
Budding, E. and Ardabili, Y. R.: 1978,Astrophys. Space Sci. 59, 19.
Demircan, O.: 1977,Astrophys. Space Sci. 52, 189 (Paper XIII).
Demircan, O.: 1978,Astrophys. Space Sci. 59, 313 (Paper XXI).
Demircan, O.: 1979a,Astrophys. Space Sci. (in press).
Demircan, O.: 1979b,Astrophys. Space Sci. (in press).
Dini, U.: 1880,Serie di Fourier, Pisa.
Erdélyi, A., Magnus, W., Oberhettinger, F. and Tricomi, F. G.: 1954,Tables of Integral Transforms, II, McGraw-Hill Publ. Co., New York.
Kopal, Z.: 1975,Astrophys. Space Sci. 38, 191 (Paper V).
Kopal, Z.: 1976,Astrophys. Space Sci. 45, 269 (Paper IX).
Kopal, Z.: 1977a,Astrophys. Space Sci. 46, 87 (Paper X).
Kopal, Z.: 1977b,Astrophys. Space Sci. 51, 439 (Paper XII).
Lommel, E. C. J. von,: 1868,Studien über die Bessel'schen Functionen, Leipzig.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Demircan, O. Fourier techniques for an analysis of eclipsing binary light curves: III. Astrophys Space Sci 62, 189–201 (1979). https://doi.org/10.1007/BF00643912
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00643912