Results 171 to 180 of about 238,671 (290)
The properties of slim accretion disks, while crucial for our understanding of black hole growth, have yet to be studied extensively observationally. We analyze the multiepoch broadband spectral energy distribution of the changing-look active galactic ...
Ruancun Li+3 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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Cosmic X-ray Background from Early Active Galactic Nuclei [PDF]
A. A. Zdziarski
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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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Quasiperiodic oscillations (QPOs) have been widely observed in black hole X-ray binaries (BHBs), which often exhibit significant X-ray variations. Extensive research has explored the long-term evolution of the properties of QPOs in BHBs.
Ruisong Xia, Hao Liu, Yongquan Xue
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Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
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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The X-ray quasiperiodic oscillation (QPO) is a remarkable form of variability in systems of compact object accretion. RE J1034+396, harboring the most significant X-ray QPO in active galactic nuclei (AGNs), is the most noteworthy source for in-depth ...
Ruisong Xia, Hao Liu, Yongquan Xue
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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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