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Fig. 10.
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HR diagram for components of studied binaries. Upper panel: models of stellar evolution according to Claret (2019) for masses of 1.8, 2.0, 2.5, and 3.0 M⊙ are plotted. Bottom panel: isochrones calculated for ages from 2 × 108 to 109 yr according to CMD 3.7 and PARSEC 2.0 models are given.
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