Fig. 4.From: Thermal and hydrostatic structure of the protoplanetary disks: Influences of wind strengths, mass distributions, and stellar wind velocity lawsSpectral energy distributions for 3 protoplanetary disks which have the surface temperature presented in Fig. 2(a). Mach mass loss times are equal to 1 × 1012, 1 × 1010, and 1 × 108 yr.Back to article page