Adiabatic Index in Fluid Models of Collisionless Black Hole Accretion
Models of highly sub-Eddington accretion onto black holes commonly use a single-fluid model for the collisionless, near-horizon plasma. These models must specify an equation of state.
Charles F. Gammie
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Active galactic nuclei dust tori at low and high luminosities [PDF]
S. F. Hönig, T. Beckert
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Revision of Two-temperature Magnetically Arrested Flows onto a Black Hole
We revisit the radiative properties of 3D general relativistic magnetohydrodynamics (GRMHD) two-temperature magnetically arrested disk (MAD) models in which electrons are heated by a magnetic turbulent cascade.
M. Mościbrodzka
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Search for High-excitation Emission Lines from a Quasar-scale Active Nucleus in Arp 220
The late-stage galaxy merger and prototypical ultraluminous infrared galaxy (ULIRG) Arp 220 is probed using the JWST Mid Infrared Instrument medium-resolution spectrometer to search for multiple diagnostic active galactic nuclei (AGN) emission lines in ...
Charles E. Goldberg+10 more
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Discovery of spectacular quasar-driven superbubbles in red quasars. [PDF]
Shen L+9 more
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Spectral Energy Distribution Models for Low-luminosity Active Galactic Nuclei in LINERs
Low-luminosity active galactic nuclei (LLAGNs) represent the bulk of the AGN population in the present-day universe and they trace the low-level accreting supermassive black holes. In order to probe the accretion and jet physical properties in LLAGNs as a class, we model the broadband radio to X-rays spectral energy distributions (SEDs) of 21 LLAGNs in
Nemmen, Rodrigo+2 more
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Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S+7 more
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The anticorrelation between the hard X-ray photon index and the Eddington ratio in low-luminosity active galactic nuclei [PDF]
Minfeng Gu, Xinwu Cao
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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.
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Changing-look quasars (CLQs) exhibit dramatic variability in broad emission-line fluxes on short timescales. This behavior is challenging to many models of the quasar broad-line region, due in large part to the short transition times between high and low
Laura Duffy+7 more
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