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

The mass-loss rates Ṁ provided for the Wolf-Rayet (WR) stars in Table 2 in the original paper were derived from the transformed radii Rt. While Rt is correctly defined in the paper (Eq. (2)), an incorrect exponent was implemented in the script used to calculate them (3/2 instead of 2/3). As a consequence, the Ṁ values, Fig. 22, and the coefficients given in Table 5 in the original paper for the Ṁ relations (Eq. (6)) are impacted. Tables 1 and 2 in this corrigendum list the revised values, and Fig. 1 shows the revised version of Fig. 22 in the original paper. Moreover, a typo pertaining to the Rt value of BAT99 119 is corrected.