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Fig. 9

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Binary light curve solutions of HD 51844. Left panel: the binary light curve of HD 51844 after the removal of the pulsational variation (red) and the best solution when both stars have radiative atmosphere (black). The residual curve is also plotted in the bottom. Right panel: comparison of the radiative solution to the “best-fit” light curve solution for a convective secondary atmosphere.

This figure is made of several images, please see below:

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