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Fig. 4
Temperature profiles of a neutron star with MB = 1.6 solar masses, spinning-down (due to magnetic braking) from an initial frequency of 500 Hz and with K = 1.0 × 10-15 s. The figures above represent different stages of the thermal evolution of the neutron star, i.e. 0.1 (a), 10 (b), 25 (c) , and 105(d) years after birth.
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