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Fig. 3.

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Comparison between our derived properties and MIST stellar models for V1044 Cen for various masses. The left panels show the radius (upper) and effective temperature (lower) as a function of age, for various stellar masses, with the derived quantities indicated with the black lines and the grey shaded regions. For the radius, we also show the Roche lobe radius for a circular orbit (red dotted line) and at periastron for e = 0.16 (purple dotted line). The right panel shows the H-R diagram, with the inset showing the whole region. Our derived quantities are indicated with the black point and the error bars.

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