Gapless neutron superfluidity from vortex pinning explains late-time cooling of KS 1731-260 and MXB 1659-29 without requiring suppression of superfluidity.
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Gapless neutron superfluidity can explain the late time cooling of transiently accreting neutron stars
Gapless neutron superfluidity from vortex pinning explains late-time cooling of KS 1731-260 and MXB 1659-29 without requiring suppression of superfluidity.