Abstract
The main aim of this paper will be to develop explicit form of the moments of the light curvesA 2m(r 1,r 2,i) required for the solution for the geometrical elementsr 1,2 andi of eclipsing systems exhibiting annular eclipses (Sections 2 and 3), as well as partial eclipses (Section 4).
In the concluding Section 5 we shall demonstrate that — regardless of the type of eclipse and distribution of brightness on the apparent disc of the eclipsed star, or indeed of the shape of the eclipsing as well as eclipsed components — the momentsA 2m satisfy certain simple functional equations — a fact which relates them to other classes of functions previously studied in applied mathematics.
Similar content being viewed by others
References
Appell, P.: 1880,Ann. Ecole Normale, Paris, (2)9, 119.
Kopal, Z.: 1947Harvard Obs. Circ., No. 450.
Kopal, Z.: 1959,Close Binary Systems, Chapman-Hall and John Wiley, London and New York.
Kopal, Z.: 1975a,Astrophys. Space Sci. 34, 431 (Paper I).
Kopal, Z.: 1975b,Astrophys. Space Sci. 35, 159 (Paper II).
Kopal, Z.: 1975c,Astrophys. Space Sci. 35, 171 (Paper III).
Kopal, Z.: 1975d,Astrophys. Space Sci. 36, 227 (Paper IV).
Kopal, Z.: 1975e,Astrophys. Space Sci. 38, 191 (Paper V).
Kopal, Z., Markellos, V., and Niarchos, P.: 1976,Astrophys. Space Sci. 40, 183 (Paper VI).
Truesdell, C.: 1948,A Unified Theory of Special Functions, (Ann. Math. Stud., No. 18), Princeton Univ. Press, Princeton, N.J.
Tsesevich, V. P.: 1939,Bull. Astron. Inst. USSR Acad. Sci., No. 45.
Tsesevich, V. P.: 1940,Bull. Astron. Inst. USSR Acad. Sci., No. 50.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kopal, Z. Fourier analysis of the light curves of eclipsing variables, VIII. Astrophys Space Sci 40, 461–481 (1976). https://doi.org/10.1007/BF00640457
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00640457