000001908 001__ 1908
000001908 005__ 20160701171655.0
000001908 037__ $$aASTROimport-65
000001908 100__ $$aBlomme, R.
000001908 245__ $$aStellar winds of massive stars driven by radiation pressure and turbulence
000001908 260__ $$c1991
000001908 520__ $$aIn a radiatively driven wind model, the dynamical effect of turbulence is included. Models are calculated for core hydrogen burning stars, luminous blue variables and a Wolf-Rayet star. For all these models the addition of turbulence either has little effect or else leads to a large temperature increase which is contrary to observational evidence. Turbulence therefore cannot explain the discrepancies between the observed and theoretical terminal velocities for O-type stars. Neither can it explain the large mass loss rates observed in luminous blue variables (during their eruptive phase) or Wolf-Rayet stars. 
000001908 700__ $$a Vanbeveren, D.
000001908 700__ $$a van Rensbergen, W.
000001908 773__ $$c479-487$$pAstronomy and Astrophysics$$v241$$y1991
000001908 85642 $$ahttp://esoads.eso.org/abs/1991A%26A...241..479B
000001908 905__ $$apublished in
000001908 980__ $$aREFERD