期刊
PHYSICAL REVIEW LETTERS
卷 98, 期 7, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.98.071101
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We show the existence of a strong trend between neutron star (NS) surface temperature and the dipolar component of the magnetic field extending through three orders of field magnitude, a range that includes magnetars, radio-quiet isolated neutron stars, and many ordinary radio pulsars. We suggest that this trend can be explained by the decay of currents in the crust over a time scale of similar to 10(6) yr. We estimate the minimum temperature that a NS with a given magnetic field can reach in this interpretation.
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