High Energy Radiation from Neutron Star Binaries

@inproceedings{CatoneHighER,
  title={High Energy Radiation from Neutron Star Binaries},
  author={Monteporzio Catone}
}
  • Monteporzio Catone
This paper surveys our current knowledge of the hard X-ray emission properties of old ac-creting neutron stars in low mass X-ray binaries. Hard X-ray components extending up to energies of a few hundred keV have been clearly detected in sources of both the Atoll and Z classes. The presence and characteristics of these hard components are discussed in relation to source properties and state. An overall anticorrelation between the fraction luminosity in hard X-rays and mass accretion rate is… CONTINUE READING

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