Fig. 3.From: Thermal and hydrostatic structure of the protoplanetary disks: Influences of wind strengths, mass distributions, and stellar wind velocity lawsThe disk heights, zs, for the five cases of t*/ β (panel(a)) and the power-law index, q, i.e., dln zs/d ln r (panel(b)). In the figure, the symbol n has the same meaning as in Fig. 2.Back to article page