Abstract
The paper is devoted to the actual problematics in the determination of orbital and physical parameters of active CB on the basis of the interpretation of photometric observations. One solves the problem in two stages: by obtaining a synthetic light curve in the case when the parameters of the corresponding CB model (Djurašević, 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 the observations is achieved (inverse problem) (Djurašević, 1992b). In this paper, the above procedure is applied to a particular case of an interpretation of CB light curves WZ Cep and FT Lupi.
Similar content being viewed by others
References
Djurašević G.: 1991,Publ. Obs. Astron, Belgrade No.42, 1–215.
Djurašević G.: 1992a,Astroph. Space Science 196, 241–265.
Djurašević G.: 1992b,Astroph. Space Science 197, 17–34.
Hoffmann, M.: 1984,Veröff. der Astron. Inst. Bonn No.96.
Hilditch, R. W.et al.: 1984,Monthly Not. Roy. Astr. Soc. 208, 135.
Kalužny, J,: 1986a,Acta Astron. 36, 105.
Kalužny, J,: 1986b,Acta Astron. 36, 113.
Lipari, S. L., and Sistero, R. F.: 1983,I.B.V.S. No.2422.
Lipari, S. L., and Sistero, R. F.: 1986,Monthly Not. Roy. Astr. Soc. 220, 883.
Marquardt, D. W.: 1963,J. Soc. Ind. Appl. Math. 11, No. 2, 431.
Mauder, H.: 1982, in: Z. Kopal and J. Rahe (eds.),Binary and Multiple Stars as Tracers of Stellar Evolution, IAU Coll.69, 275.
Mauder, H.: 1984,The Messenger 35, 38.
Morton, D. C. and Adams, T. F.: 1968,Astroph. J. 151, 611.
Wilson, R. E. and Devinney, E. J.: 1971,Astroph. J. 166, 605.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Djuraševic, G. An analysis of close binaries (CB) based on photometric measurements (VI). Astrophys Space Sci 206, 145–159 (1993). https://doi.org/10.1007/BF00658390
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00658390