An Analysis of Close Binaries Based on Photometric Measurements - Part Six - an Interpretation of CB Lightcurves Wz-Cephei and Ft-Lupi by Using the Inverse-Problem Method

Details An Analysis of Close Binaries Based on Photometric Measurements - Part Six - an Interpretation of CB Lightcurves Wz-Cephei and Ft-Lupi by Using the Inverse-Problem Method An Analysis of Close Binaries Based on Photometric Measurements - Part Six - an Interpretation of CB Lightcurves Wz-Cephei and Ft-Lupi by Using the Inverse-Problem Method

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.206..145d&link_type=abstract

Astrophysics and Space Science, Volume 206, Issue 1, pp.145-159

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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