Fig. 2.

Overview of the thermal and pressure profiles of our early solar nebula model compared to previous simulations. ProDiMo values are for a 0.03 M⊙ disk. Values from Lewis (1974), Cameron (1995), and Willacy et al. (1998) are taken from Fig. 1 of Fegley (1999); the first one is extrapolated to a lower radius than in the original work; the temperature and pressure values of Hersant et al. (2001) and Davis (2005a) are extracted from their figures.
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