Apsidal motion in massive eccentric binaries in NGC 6231 - The case of HD 152219

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Fig. 14.

Evolution as a function of stellar age of the contributions and to the weighted-average mean of the internal structure constants k_2, 1 and k_2, 2 (to which the empirical correction Eq. (22) has been applied) for the models presented in Fig. 13.

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