White dwarfs in the building blocks of the Galactic spheroid

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Fig. B.4

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Mass of the brightest star in the binary system versus the period of that system in days, for unresolved binary halo WDs in the solar neighbourhood that can be observed with Gaia (G < 20). Colours for age and metallicity values are the same as in Figs. B.1, B.2, and B.5.

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