1908 20160701171655.0 ASTROimport-65 Blomme, R. 1991 Stellar winds of massive stars driven by radiation pressure and turbulence In a radiatively driven wind model, the dynamical effect of turbulence is included. Models are calculated for core hydrogen burning stars, luminous blue variables and a Wolf-Rayet star. For all these models the addition of turbulence either has little effect or else leads to a large temperature increase which is contrary to observational evidence. Turbulence therefore cannot explain the discrepancies between the observed and theoretical terminal velocities for O-type stars. Neither can it explain the large mass loss rates observed in luminous blue variables (during their eruptive phase) or Wolf-Rayet stars. Vanbeveren, D. van Rensbergen, W. Astronomy and Astrophysics 241 1991 479-487 http://esoads.eso.org/abs/1991A%26A...241..479B published in REFERD