The Wolf–Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud - Spectroscopy, orbital analysis, formation, and evolution

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201935684e]

Fig. 21.

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Histogram of v_eq for the 16 OB-type companions of WN stars with constrained v sin i (Table 2) and i (Table 3), assuming an alignment of the rotational and orbital axes. Upper limits contribute equally to all lower bins, hence the fractional counts.

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