Proceedings of the International Astronomical Union
The nearby compact object RX J1856.5−3754 may be a paradigm for the vast majority of neutron stars. Its spectral energy distribution lacks any non-thermal continuua or lines. Study of the thermal surface has provided insights into the surface and interior properties of neutron stars. We report on attempts to model the spectrum. Non-magnetic heavy metal atmospheres reproduce the overall spectral energy distribution, but not the lack of absorption lines.
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