Fig. 9.
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Comparison of the observed period and the theoretical period of a binary in which one star fills its Roche lobe (see Sect. 6.3.4). Different marker shapes correspond to different types of stars, and colours represent spectral classes (using our classification when available, and Gaia’s otherwise). Sources that lie, based on SHBoost values, within our defined HG parameter space are highlighted with circles.
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