Fig. 2
Thermal evolution with rotochemical heating. All curves correspond to stars with mass M = 1.4 M⊙, A18 + δυ + UIX* EOS (which allows only for modified Urca reactions), initial temperature T = 108 K, and magnetic field B = 108 G. The solid lines show the evolution of the internal temperature T and the chemical imbalance ηnpe, and the dotted line shows the passive cooling.
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