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Fig. 5
Column gas density in the disk wind between the star and an arbitrary point on the disk surface. Here we used our disk wind models for the Herbig Ae star HD 163296 (MWC 275; black lines) and Herbig Be star HD 98922 (red lines; see text). The disk is flared with p = 9/8 (dashed lines) and p = 5/4 (solid lines).
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