Relativistic reflection modeling in AGN and related variability from PCA: a brief review
X-ray observations of active galactic nuclei (AGNs) reveal relativistic reflections from the innermost regions of accretion disks, which contain general-relativistic footprints caused by spinning supermassive black holes (SMBH). We anticipate the spin of a SMBH to be stable over the human timeframe,...
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| Format: | Article |
| Language: | English |
| Published: |
Frontiers Media S.A.
2024-10-01
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| Series: | Frontiers in Astronomy and Space Sciences |
| Subjects: | |
| Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2024.1479301/full |
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