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The Super-Massive Black Hole close environment in Active Galactic Nuclei
W. Alston
, M. Giustini
, P. O. Petrucci
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Centre of Data Innovation Research
Research output
:
Chapter in Book/Report/Conference proceeding
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Chapter
127
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Dive into the research topics of 'The Super-Massive Black Hole close environment in Active Galactic Nuclei'. Together they form a unique fingerprint.
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Keyphrases
Close Environment
100%
Supermassive Black Holes (SMBHs)
100%
Active Galactic nuclei
100%
X-ray
60%
Energy Release
40%
Accretion Flow
20%
High-energy Emissions
20%
Deep Potential
20%
Efficient Mechanism
20%
Optically Thick
20%
Gravitational Radius
20%
Physical Properties
20%
Absorption Mechanism
20%
High Energy
20%
Radiative Mechanisms
20%
Rest Mass Energy
20%
Accretion Processes
20%
Electromagnetic Spectrum
20%
Emission Mechanism
20%
Potential Well
20%
Optically Thin Plasma
20%
Ejection Mechanism
20%
UV Emission
20%
Corona
20%
Physics
Black Hole
100%
Active Galactic Nuclei
100%
X Ray
40%
Electromagnetic Spectra
20%
Schwarzschild Radius
20%
Blood Plasma
20%