Powering Anomalous X-ray Pulsars by Neutron Star Cooling
arXiv:astro-ph/9708179 · doi:10.1086/310964
Abstract
Using recently calculated analytic models for the thermal structure of ultramagnetized neutron stars, we estimate the thermal fluxes from young ( yr) ultramagnetized ( 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 g/cm. The total mass of this insulating layer is .
8 pages, 1 figure, to appear in Ap.J. Letters (one reference entry corrected, no other changes)
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Cited by in corpus (48)
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