Fig. 2.From: Thermal and hydrostatic structure of the protoplanetary disks: Influences of wind strengths, mass distributions, and stellar wind velocity lawsTemperature distributions of the disk for the five cases of t*/ β from 1 × 108to 1 × 1012 yr (panel (a)). We also show the corresponding power-law index p defined as p = −dlnT/dln r in panel (b). In the figure, the index n represents the case of t*/ β = 1 × 10n yr.Back to article page