Supermassive Black Holes in Early-Type Galaxies: Relationship with Radio Emission and Constraints on the Black Hole Mass Function [PDF]
A. Franceschini+2 more
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Dynamics Around Supermassive Black Holes: Extreme-mass-ratio Inspirals as Gravitational-wave Sources
Supermassive black holes and their surrounding dense stellar environments nourish a variety of astrophysical phenomena. We focus on the distribution of stellar-mass black holes around the supermassive black hole and the consequent formation of extreme ...
Barak Rom+3 more
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Phenomenological Analogies in Black Hole Systems of all Masses
I review the progress made on the physics of relativistic jets from black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago.
Mirabel, I. F.
core +2 more sources
New Estimates of the Spin and Accretion Rate of the Black Hole M87*
In this Letter, we use the imaging results of M87* from the Event Horizon Telescope (EHT) to calculate the rotational velocity of the inner edge of the accretion disk and find a value of ∼0.14 c .
Michael Drew+4 more
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Super-Eddington Accretion in Quasars
This review provides an observational perspective on the fundamental properties of super-Eddington accretion onto supermassive black holes in quasars.
Paola Marziani+7 more
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Quasiperiodic oscillations (QPOs) are very common in black hole accretion systems that are seen from the modulations in luminosity. Many supermassive black hole sources (e.g., RE J1034+396, 1H 0707-495, MCG-6-30-15, 1ES 1927+654, Sgr A*) have been ...
Indu K. Dihingia, Yosuke Mizuno
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Evidence for Supermassive Black Holes in Active Galactic Nuclei from Emission-Line Reverberation [PDF]
B. M. Peterson, Amri Wandel
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Tidal Disruption of a Solar‐Type Star by a Supermassive Black Hole [PDF]
Shai Ayal, Mario Livio, Tsvi Piran
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The Effect of the Self‐Gravity of Gas on Gas Fueling in a Barred Galaxy with a Supermassive Black Hole [PDF]
Hiroyuki Fukuda, Asao Habe, Keiichi Wada
openalex +1 more source
Simulating ULXs and Blazars as GRMHD Accretion Flows Around a Black Hole
General relativistic magnetohydrodynamic (GRMHD) simulations have been instrumental in our understanding of high-energy astrophysical phenomena over the past two decades.
Mayank Pathak, Banibrata Mukhopadhyay
doaj +1 more source