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Earth, Planets and Space
Fig. 9. | Earth, Planets and Space

Fig. 9.

From: Thermal and hydrostatic structure of the protoplanetary disks: Influences of wind strengths, mass distributions, and stellar wind velocity laws

Fig. 9.

Disk temperatures predicted by various models. Solid line denotes our result for the case of t*/β = 1 × 1010 yr. Dashed line and dotted line are temperature distributions of models of K70 and CG97, respectively. To compare the models under the same conditions, the temperature of K70 and that of CG97 are recalculated by using the parameters of the central star, M* = 1M☉, R* = 2R☉, and T* = 4000 K, after ours.

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