Fig. A.1
Comparison of T/μ (in K) as calculated from the heating/cooling terms in our thermal-chemical models (red solid curves) with the same ratio as assumed in the dynamical MHD solutions of Casse & Ferreira (2000), in dashed green, for the 1 AU streamline and 3 stars of differing accretion properties. Note that in the dynamical solution, Tdyn is calculated assuming a fully ionised gas, with μdyn = 0.5.
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