An observational study of rotation and binarity of Galactic O-type runaway stars

Open Access

Fig. B.1.

$V_{PEC}^{2 D}$ $V_{\mathrm{PEC}}^{\mathrm{2D}}$ distributions for the normal stars (unfilled black bars) and runaway stars (filled blue bars) with a bin size of 5 km s⁻¹, for the rotation sample (top), the fast rotators (middle), and the slow rotators (bottom).

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