Fig. 9.
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v sin i distributions of non-OBe main-sequence systems together with single SB1 and SB2 systems. The sample sizes are as indicated in the insets. In the SB2 panel (lower right), the v sin i distribution of the eclipsing systems (ECL) in BLOeM is also shown (dashed line). The histogram bin size is 20 km s−1. The total of main-sequence sources is greater than the sum of single SB1 and SB2 as some main-sequence sources have unclear multiplicity designations, as discussed at the beginning of Sect. 4.
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