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Close Binaries in the 21st Century: New Opportunities and Challenges
Eclipsing binary stars are gratifying objects because of their unique geometrical properties upon which all important physical parameters such as masses, radii, temperatures, luminosities and distance may be obtained in absolute scale. This poses strict demand on the model to be free of systematic effects that would influence the results later used for calibrations, catalogs and evolution theory. We present an objective scheme of obtaining individual temperatures of both binary systemdoi:10.1007/978-1-4020-5027-5_86 fatcat:kqxxhquj7jfipgfxypaadsih6q