Fig. 11
Illustration comparing the radiative line force with other terms in the momentum equation. The model parameters are similar to those of ζ Puppis; Teff = 41 000 K and M⊙ = 1.7 × 10-6 M⊙ yr-1. The right-hand plot illustrates the sensitivity of the line force to the adopted microturbulent velocity around the sonic point. Below 10 km s-1 hydrostatic equilibrium is valid.
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