Fig. 12.
Cumulative distributions of the projected rotational velocities of the massive single and binary populations in the 30 Doradus region. Red: VFTS “presumably” single stars (Ramírez-Agudelo et al. 2013), Green: VFTS primaries in detected binary system (most luminous components, Ramírez-Agudelo et al. 2015); Blue: primaries in the present 31 SB2 TMBM sample (=currently most massive component, this work); Magenta: secondaries in the present 31 SB2 TMBM sample (=currently least massive component, this work).
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