Spectral Lines from Rotating Neutron Stars

@article{Ozel2002SpectralLF,
  title={Spectral Lines from Rotating Neutron Stars},
  author={Feryal Ozel and Dimitrios Psaltis},
  journal={The Astrophysical Journal},
  year={2002},
  volume={582}
}
The line profiles from rotating neutron stars are affected by a number of relativistic processes such as Doppler boosts, strong self-lensing, frame dragging, and the differential gravitational redshift arising from the stellar oblateness. In this Letter, we calculate line profiles, taking into account the first two effects; this approach is accurate for rotation rates less than the breakup frequency. We show that the line profiles are not only broadened and weakened but are also significantly… 

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