1884 20160701171654.0 10.1007/BF01091157 DOI ASTROimport-41 Runacres, M. 1994 The infrared and radio continuum of OB-stars The infrared and radio continuum fluxes of a number of OB-stars are compared to theoretical models. This gives us information about the mass loss rates and the structure of the stellar wind. The more extreme O-star zeta Pup appears to show an effect of clumping in its continuum flux. Blomme, R. Astrophysics and Space Science 221 1994 249-257 http://esoads.eso.org/abs/1994Ap%26SS.221..249R published in REFERD