On the Magnetic Field of the Ultraluminous X-Ray Pulsar M82 X-2

@article{Xu2017OnTM,
  title={On the Magnetic Field of the Ultraluminous X-Ray Pulsar M82 X-2},
  author={Kun Xu and Xiang-Dong Li},
  journal={The Astrophysical Journal},
  year={2017},
  volume={838},
  pages={98}
}
The discovery of the ultraluminous X-ray pulsar M82 X-2 has stimulated lively discussion on the nature of the accreting neutron star. In most of the previous studies the magnetic field of the neutron star was derived from the observed spin-up/down rates based on the standard thin, magnetized accretion disk model. However, under super-Eddington accretion the inner part of the accretion disk becomes geometrically thick. In this work we consider both radiation feedback from the neutron star and… Expand

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