Cosmic X-ray Background from Early Active Galactic Nuclei [PDF]
A. A. Zdziarski
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Active galactic nuclei (AGN) emit radiation via accretion across the entire energy spectrum. While the standard disk and corona model can somewhat describe this emission, it fails to predict specific features such as the soft X-ray excess, the short-term
Kriti Kamal Gupta +22 more
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Penrose pair production as a power source of quasars and active galactic nuclei
M. Kafatos, D. Leiter
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Thick tori around active galactic nuclei: a comparison of model predictions with observations of the infrared continuum and silicate features [PDF]
G. L. Granato, L. Danese
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Low-ionization active galactic nuclei - X-ray or shock heated?
J. P. Halpern, J. E. Steiner
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Anisotropic induced Compton scattering - Constraints on models of active galactic nuclei [PDF]
P. Coppi, R. D. Blandford, M. J. Rees
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On the two states of CYG X-1 and related sources [PDF]
A model for active galactic nuclei (AGN), employing quasi-spherical accretion onto a black hole, when scaled down to solar mass objects, provides a straightforward account of the bimodal spectral behavior of Cyg X-1 and the other galactic black hole ...
Kazanas, D.
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Evolution of self-gravitating accretion disks in active galactic nuclei
Isaac Shlosman, Mitchell C. Begelman
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Implications of particle acceleration in active galactic nuclei for cosmic rays and high energy neutrino astronomy [PDF]
Á. Szabó, R. J. Protheroe
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Accretion disks and periodic outbursts of active galactic nuclei
D. N. C. Lin, G. A. Shields
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