Generally Applicable Formalism for Modeling the Observable Signatures of Inflows, Outflows, and Moving Coronal Plasma Close to Kerr Black Holes
Author:
Funder
NASA
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/abc32f/pdf
Reference66 articles.
1. The Polarization of X-Rays from Warped Black Hole Accretion Disks
2. Testing the Kerr Black Hole Hypothesis Using X-Ray Reflection Spectroscopy and a Thin Disk Model with Finite Thickness
3. The Contribution of Particle Impact to the Production of Fe Kα Emission from Accreting Black Holes
4. Rotating Black Holes: Locally Nonrotating Frames, Energy Extraction, and Scalar Synchrotron Radiation
5. The X-Ray Polarization of the Accretion Disk Coronae of Active Galactic Nuclei
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1. Formation of Magnetically Truncated Accretion Disks in 3D Radiation-transport Two-temperature GRMHD Simulations;The Astrophysical Journal Letters;2022-08-01
2. New Constraints on the Spin of the Black Hole Cygnus X-1 and the Physical Properties of its Accretion Disk Corona;The Astrophysical Journal;2022-07-01
3. Electromagnetic signatures of strong-field gravity from accreting black-holes;Advances in Space Research;2022-01
4. Comptonization by reconnection plasmoids in black hole coronae I: Magnetically dominated pair plasma;Monthly Notices of the Royal Astronomical Society;2021-09-08
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