000002426 001__ 2426
000002426 005__ 20160701171705.0
000002426 037__ $$aASTROimport-583
000002426 100__ $$aBlomme, R.
000002426 245__ $$aModels for stellar wind of early-type stars.
000002426 260__ $$c1992
000002426 520__ $$aThe radiatively driven wind theory does not correctly predict the observed values of the terminal velocity and mass loss rate for O and early B-type stars. Hoping to explain this discrepancy the authors investigated how sensitive the theoretical predictions are to errors in the oscillator strengths. The results show that the stellar wind dynamics is quite sensitive to changes in the oscillator strengths for the iron-group elements. For some stars the mass loss rate increases by a factor of 2, bringing them much closer to the observed rates. Unfortunately at the same time the terminal velocity also increases, making the discrepancy of that parameter with the observations even larger. 
000002426 773__ $$c241-246$$pRevista Mexicana de Astronomia y Astrofisica, vol. 23$$v23$$y1992
000002426 85642 $$ahttp://esoads.eso.org/abs/1992RMxAA..23..241B
000002426 905__ $$apublished in
000002426 980__ $$aNONREF