Fig. 3.

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Distribution of the 318 Galactic O-type stars in a modified Hunter diagram, using He abundance instead of nitrogen on the y-axis. The fractions of He-rich stars in the slow- and fast-rotating subsamples are indicated, assuming v sin i = 200 km s−1 as the dividing threshold. ON, SB1, and RW stars are indicated with red small circles, blue crosses, and grey circles, respectively.
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