Fig. G.4.
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Predicted distribution of the orbital velocities υorb, WR of the WR stars in the WR+O binaries. Three subpopulations are identified, which are featured by Porb > 20 days (blue), Porb < 20 days and MWR/MO > 0.6 (purple), and Porb < 20 days and MWR/MO < 0.6 (observed region, red). The numbers of WR+O binaries correspond to each subpopulations are indicated by the text in the legend.
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