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Fig. 8


Results for the ρ0 and n distributions of the sample of Be stars studied by Vieira et al. (2017). The main panel shows the probability density (gray scale contours), while the upper and right panels show the distributions for the individual parameters. The contour values correspond to the probability density levels. Superimposed as filled circles are the results of Vieira et al. for individual stars (colors indicate the stellar effective temperatures computed by Frémat et al. 2005). Over-plotted as yellow star symbols are the results for the stars studied in this work.

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