WR 146 - observing the OB-type companion

We present new radio and optical observations of the colliding-wind system WR 146 aimed at understanding the nature of the companion to the Wolf-Rayet (WR) star and the collision of their winds. The radio observations reveal emission from three components: the WR stellar wind, the non-thermal wind-w ind interaction region and, for the first time, the stellar wind of the OB companion. This provides the unique possibility of determining the mass-los s rate and terminal wind velocity ratios of the two winds, independent of d istance. Respectively, these ratios are 0.20 +/- 0.06 and 0.56 +/- 0.17 for the OB-companion star relative to the WR star. A new optical spectrum indi cates that the system is more luminous than had been believed previously. W e deduce that the 'companion' cannot be a single, low-luminosity O8 star as suggested previously, but is either a high-luminosity O8 star, or possibly an O8+WC binary system.