A relativistically broadened O viii Lyα line in the ultracompact X‐ray binary 4U 0614+091

@article{Madej2010ARB,
  title={A relativistically broadened O viii Ly$\alpha$ line in the ultracompact X‐ray binary 4U 0614+091},
  author={Oliwia Madej and Peter G. Jonker and Andrew C. Fabian and Ciro Pinto and Frank Verbunt and Jelle de Plaa},
  journal={Monthly Notices of the Royal Astronomical Society: Letters},
  year={2010},
  volume={407}
}
Ultra-compact X-ray binaries consist of a neutron star or black hole that accretes material from a white dwarf-donor star. The ultra-compact nature is expressed in very short orbital periods of less than 1 hour. In the case of 4U 0614+091 oxygen-rich material from a CO or ONe white dwarf is flowing to the neutron star. This oxygen- rich disc can reflect X-rays emitted by the neutron star giving a characteristic emissio n spectrum. We have analyzed highresolution RGS and broad band EPIC spectra… Expand

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