Absolute Properties of Binary Stars

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Scientific paper

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Scientific paper

Our goals are (1) to determine the internal structure of stars over a wide range of masses in order to make critical comparisons with theoretical models, (2) to determine accurately other fundamental properties of main-sequence stars in order to make critical comparisons with theoretical models. We propose to do this by observing selected eclipsing binary stars. This request is for the coude-feed time to measure accurate radial velocity curves. The proposers are obtaining accurate light curves with an automatic observing system at the University of Arkansas-Fayetteville.

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