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Fig. 6

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Mass-radius diagram of the subsystem WDS 08263–3904 Aab. Filled circles with error bars represent the components, whose positions are compared with the models of Lejeune & Schaerer (2001) for solar composition. Isochrones corresponding to log τ = 6.5 and log τ = 7.0 are plotted in continuous and dashed lines, respectively.

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