Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.206..129d&link_type=abstract
Astrophysics and Space Science, Volume 206, Issue 1, pp.129-144
Astronomy and Astrophysics
Astrophysics
Scientific paper
The author considers the current problematics in the determination of the orbital and physical parameters for active close binaries (CB) of W Ser type based on the interpretation of photometric observations. In the particular case one analyses the light curves of CB RX Cas in the framework of the accretion-disc model explained in the second paper of this series (Djurašević, 1992a). The change of the light curves with that of the system's physical-activity phase is analysed and the orbital and physical parameters of the system are determined for the maximum, minimum and the transition regime of the physical activity by applying the inverse-problem method described in the third paper of the series (Djurašević, 1992b). In the paper a graphical illustration of the solutions obtained is also given.
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