Fig. 7
Steady-state velocity profile (solid) of the stellar model used in this paper. The grey shading marks the region of high photospheric continuum optical depth τRos ≥2∕3, with R(τRos = 2∕3) ≈ 3.5R⋆. In crossed-dashed line a vβ velocity fit to the optically thin region is given, which was extrapolated to the optically thick region to recover the stellar core radius.
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