Results 141 to 150 of about 77,605 (280)
Abstract Accurate representation of aerosol size distributions and total number concentrations is critical for evaluating particle impacts on climate, clouds, and public health. An Advanced Particle Microphysics model (APM) has been integrated into the USEPA's Community Multiscale Air Quality Modeling System (CMAQ) to improve its representation of ...
Jingbo Mao+7 more
wiley +1 more source
Jets in Active Galactic Nuclei
26 pages, 9 figures, To appear in Belloni, T. (ed.): The Jet Paradigm - From Microquasars to Quasars, Lect. Notes Phys. 794 (2009)
openaire +3 more sources
Effects of superradiance in active galactic nuclei
ABSTRACT A supermassive black hole (SMBH) at the core of an active galactic nucleus (AGN) provides room for the elusive ultra-light scalar particles to be produced through a phenomenon called superradiance. This phenomenon produces a cloud of scalar particles around the black hole by draining its spin angular momentum.
Priyanka Sarmah+3 more
openaire +3 more sources
Varstrometry for Dual Active Galactic Nuclei Using Radio Interferometry: VaDAR with the VLBA
Multiple active galactic nuclei (multi-AGN) are a known result of galaxy mergers. Therefore, they are an important tool for studying the formation and dynamical evolution of galaxies and supermassive black holes. A novel method for the selection of multi-
Emma Schwartzman+8 more
doaj +1 more source
Cosmic X-ray Background from Early Active Galactic Nuclei [PDF]
A. A. Zdziarski
openalex +1 more source
Quasiperiodic oscillations (QPOs) in active galactic nuclei (AGNs) provide a powerful tool for probing the structure of the innermost accretion flow and corona around supermassive black holes.
Ruisong Xia+3 more
doaj +1 more source
Penrose pair production as a power source of quasars and active galactic nuclei
M. Kafatos, D. Leiter
openalex +1 more source
Anisotropic induced Compton scattering - Constraints on models of active galactic nuclei [PDF]
P. Coppi, R. D. Blandford, M. J. Rees
openalex +1 more source
XRISM Spectroscopy of Accretion-driven Wind Feedback in NGC 4151
The hottest, most ionized, and fastest winds driven by accretion onto massive black holes have the potential to reshape their host galaxies. Calorimeter-resolution X-ray spectroscopy is the ideal tool to understand this feedback mode, as it enables ...
Xin Xiang+19 more
doaj +1 more source
The radiative deceleration of ultrarelativistic jets in active galactic nuclei
Fulvio Melia, Arieh Königl
openalex +1 more source