AN ANALYSIS OF CLOSE BINARIES (CB) BASED ON PHOTOMETRIC MEASUREMENTS .6. AN INTERPRETATION OF CB LIGHT CURVES WZ CEP AND FT LUPI BY USING THE INVERSE-PROBLEM METHOD

The paper is devoted to the actual problematics in the determination o f orbital and physical parameters of active CB on the basis of the int erpretation of photometric observations. One solves the problem in two stages: by obtaining a synthetic light curve in the case when the par ameters of the corresponding CB model (Djurasevic, 1992a) are given a priori (direct problem) and by determining the parameters of the given model for which the best fit between the synthetic light curve and th e observations is achieved (inverse problem) (Djurasevic, 1992b). In t his paper, the above procedure is applied to a particular case of an i nterpretation of CB light curves WZ Cep and FT Lupi.