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arXiv · astro-ph/9708179

Powering Anomalous X-ray Pulsars by Neutron Star Cooling

Jeremy S. Heyl·Lars Hernquist
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Abstract

Using recently calculated analytic models for the thermal structure of ultramagnetized neutron stars, we estimate the thermal fluxes from young ($t\sim 1000$ yr) ultramagnetized ($B \sim 10^{15}$ G) cooling neutron stars. We find that the pulsed X-ray emission from objects such as 1E 1841-045 and 1E 2259+586 as well as many soft-gamma repeaters can be explained by photon cooling if the neutron star possesses a thin insulating envelope of matter of low atomic weight at densities $ρ< 10^{7}-10^{8}$ g/cm$^3$. The total mass of this insulating layer is $M \sim 10^{-11}-10^{-8} M_\odot$.

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BibTeXRIS

Jeremy S. Heyl, Lars Hernquist. 1997-08-30. Powering Anomalous X-ray Pulsars by Neutron Star Cooling. https://doi.org/10.1086/310964

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