Wind-momentum luminosity relationship for GHV-62024 (upper green triangle: value from Herrero et al. (2011); middle green triangle: this work; lower green triangle: this work, considering a wind terminal velocity 30% lower than quoted in Table 2) compared to data from Mokiem et al. (2007b) for the MW (red circles) and SMC (blue squares). The SMC stars cited in text were marked with an open circle. From left to right they are NGC 346-010, AzV296, AzV83 and NGC 346-001. The solid lines represent the WLR fitted by Mokiem et al. (2007b) without considering clumping for MW and SMC objects, and the black dashed line corresponds to the SMC relation shifted to Z = 0.13   Z_⊙.