Fig. 10.
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Overall observed fractions of spectroscopic binaries, runaways (including walkaways) and eclipsing binaries for all working sample of fast rotators within 3 kpc distances (according to Table 2) shown on the left. Simulated fractions of spectroscopic binaries and runaway (incl. walkaway) stars over all population of O-type fast rotators (based on the BPASS models) shown on the right.
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