Light-Time Effect in Eclipsing Binaries

Volume 19 number 1 (1990)

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Marek Wolf
Department of Astronomy and

Abstract

The role of the light-time effect in stellar studies is briefly discussed. Base on the list of published photoelectric minima, the new parameters of the third body's orbit for two well-known eclipsing binaries, TW Dra and TX Her, are derived. For each system the minimum mass of a third component is computed.