Cyclotron lines in highly magnetized neutron stars

@article{Staubert2019CyclotronLI,
  title={Cyclotron lines in highly magnetized neutron stars},
  author={Ruediger Staubert and Joachim Trumper and Eckhard Kendziorra and Dmitry Klochkov and Konstantin A Postnov and Peter Kretschmar and Katja Pottschmidt and Frank Haberl and Richard E. Rothschild and Andrea Santangelo and J{\"o}rn Wilms and Ingo Kreykenbohm and F. Furst},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Cyclotron lines, also called cyclotron resonant scattering features are spectral features, generally appearing in absorption, in the X-ray spectra of objects containing highly magnetized neutron stars, allowing the direct measurement of the magnetic field strength in these objects. Cyclotron features are thought to be due to resonant scattering of photons by electrons in the strong magnetic fields. The main content of this contribution focusses on electron cyclotron lines as found in accreting… 

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