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Fig. 1.
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Density (in g cm−3) contours of stellar wind of the star WR93b versus radius r and colatitude θ, in log scale spaced by 0.8 dex, denoted contour correspond to log(ρ)= − 11.2, for rotation Vrot = 1100 km s−1, with nonradial forces and gravity darkening.
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