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Fig. 10
Cooling curves for neutron stars with M = 1.4 M⊙ according to the BSk24 EoS model with B = 0 (solid line), 1014 G (short-dashed line), 1015 G (long-dashed line), and 1016 G (dot-dashed line). The three dotted lines result from simulations with the same three strong fields, but treated classically.
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