The Apsidal Motion Test of the Internal Stellar Structure - Comparison Between Theory and Observations
In this paper we present the main results of an extensive comparison carried out between the most modern theoretical models of stellar structure, including moderate core over- shooting and mass loss, and the best available data of apsidal motion rates for double-lined eclipsing binaries. Though stellar absolute dimensions (radii, temperatures, etc)
Claret, A. et al.
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1993