Titlebook: Language of the Stars; A Discourse on the T Zdeněk Kopal Book 1979 D. Reidel Publishing Company, Dordrecht, Holland 1979 Inclined Orbit.cel

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Special Functions of the Theory of Light Curvesof one star by another — to the first order in small quantities in terms of ‘circular’ integrals of the form (2.15) or (2.16) of Chapter II defining the . of order . and index .; while the supplementary light changes arising from the limb distortion of the eclipsing and eclipsed components were foun

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Analysis of the Light Changes in the Time Domainneous brightness of an eclipsing variable in the course of time, with the aim of deducing from them the elements of the system enumerated in the introduction. Photometric observations of such systems performed by different methods (visual, photographic, photoelectric) furnish, in general, a series o

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Analysis of the Light Changes in the Frequency-Domain: Spherical Starsthe elements of the eclipses of the two stars. In retrospect, we note that while the problem at issue does not admit of any closed (or even algebraic) solution on account of its non-linearity, it can be solved by successive approximations (the convergence of which will be discussed more fully in Cha

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Analysis of the Light Changes in the Frequency-Domain: Distorted Starsy-domain; and presented an explicit form of such an analysis appropriate for the case in which both components can be regarded as spheres. With the completion of this task the question is, however, bound to arise as to the extent to which a model consisting of spherical stars can be regarded as a sa

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Error Analysisor frequency- (Chapters V–VI) domain, we have not yet arrived at the end of their investigation; for it still remains for us to determine the . within which such elements can be specified from the available observational data. A quest of this uncertainty constitutes a point whose importance cannot b