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Fig. 4

image

Upperpanel: maximum error in the e.o.m. (triangles) and the corresponding mass-loss rate for each hydrodynamic iteration i. Lower panel: relative change in radiative acceleration between two successive NLTE iterations j − 1 and j. The vertical dotted lines mark NLTE iterations j where hydrodynamic iteration updates i are made. Both panels show results from the early O-star model in Table 1.

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