Geometric modeling of M87* as a Kerr black hole or a non-Kerr compact object

@article{Vincent2020GeometricMO,
  title={Geometric modeling of M87* as a Kerr black hole or a non-Kerr compact object},
  author={F. Vincent and M. Wielgus and M. Abramowicz and {\'E}. Gourgoulhon and J. Lasota and T. Paumard and G. Perrin},
  journal={arXiv: General Relativity and Quantum Cosmology},
  year={2020}
}
Context. The Event Horizon Telescope (EHT) collaboration recently obtained first images of the surroundings of the supermassive compact object M87* at the center of the galaxy M87. Aims. We want to develop a simple analytic disk model for the accretion flow of M87*. Compared to general-relativistic magnetohydrodynamic (GRMHD) models, it has the advantage of being independent of the turbulent character of the flow, and controlled by only few easy-to-interpret, physically meaningful parameters… Expand
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