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We propose a procedure for light-curve solution of eclipsing binary stars inthe Small Magellanic Cloud for which photometric data have been obtained in theframework of the OGLE project as well as way of determination of the globalstellar parameters on the basis of the obtained solutions, some empiricalrelations as well as the distance to the SMC. Several examples illustrate thisprocedure.

Light Curve Solutions of Eclipsing Binaries in SMC