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Cited article:

Towards self-consistent models of isolated neutron stars

J. A. Pons, J. F. Pérez-Azorín, J. A. Miralles and G. Miniutti
Astrophysics and Space Science 308 (1-4) 247 (2007)
https://doi.org/10.1007/s10509-007-9336-8

Unveiling the thermal and magnetic map of neutron star surfaces though their X-ray emission: method and light-curve analysis

Silvia Zane and Roberto Turolla
Monthly Notices of the Royal Astronomical Society 366 (3) 727 (2006)
https://doi.org/10.1111/j.1365-2966.2005.09784.x

A self-consistent model of isolated neutron stars: the case of the X-ray pulsar RX J0720.4-3125

J. F. Pérez-Azorín, J. A. Pons, J. A. Miralles and G. Miniutti
Astronomy & Astrophysics 459 (1) 175 (2006)
https://doi.org/10.1051/0004-6361:20065827

Evidence for Surface Cooling Emission in theXMM‐NewtonSpectrum of the X‐Ray Pulsar PSR B2334+61

K. E. McGowan, S. Zane, M. Cropper, W. T. Vestrand and C. Ho
The Astrophysical Journal 639 (1) 377 (2006)
https://doi.org/10.1086/497327

Enhanced cooling of neutron stars via Cooper-pairing neutrino emission

M. E. Gusakov, A. D. Kaminker, D. G. Yakovlev and O. Y. Gnedin
Astronomy & Astrophysics 423 (3) 1063 (2004)
https://doi.org/10.1051/0004-6361:20041006