Positions of the single (adopted from H14) and binary (this work) LMC WN sample on the log L − log Ṁ plane. The meaning of the colors and symbols are indicated as in Fig. 4; the binaries are denoted with a circle (see legend). Also shown are the WN3/O3 stars analyzed by Neugent et al. (2017). The projection of Eq. (6) onto the LMC metallicity and different hydrogen content, where there temperature is fixed to typical values per subtype, are plotted. We also plot the commonly used relations published by Nugis & Lamers (2000) for the LMC and for H-rich/free stars and the theoretical relation published by Vink (2017).