Comparison of the wind properties of Wd1-5 to field BHGs, BSGs (both plotted according to spectral type, with BHGs given by solid symbols), LBVs and WNLh (=Ofpe/WNL) stars. The data and references employed are summarised in Table A.1. Unfortunately, given the diverse sources employed to construct this figure, it is not possible to plot representative errors for all the objects. In all cases clumping corrected mass loss rates are used to enable direct comparison between individual objects. We estimate  yr^-1 for Wd1-5 since the errors on the clumping factor in Table 1 are conservative and once this parameter is set the mass loss rate is also determined to a high precision.