Modeling Neutron Star Atmospheres

@inproceedings{Zavlin2002ModelingNS,
  title={Modeling Neutron Star Atmospheres},
  author={E. Zavlin and George G. Pavlov},
  year={2002}
}
Models of thermal emission of neutron stars, presumably formed in their atmospheres, are needed to infer the surface temperatures, magnetic fields, chemical composition, and neutron star masses and radii from the observational data. This information, supplemented with model equations of state and neutron star cooling models, is expected to move us further in understanding the fundamental properties of the superdense matter in the neutron star interiors. The neutron star atmospheres are very… CONTINUE READING

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