Fig. A.1
Observed Hα of Be stars with both stellar absorption (dashed green lines) and total emission profiles (solid red lines) overimposed. Best fit parameters for stellar and disk synthetic profiles are reported in Table 2. The circumstellar emission have been calculated by fixing the radial density exponent (n = 3) and considering Keplerian rotation of the disk (i.e. j = 1/2).
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