activity
19972026
most citedHydrodynamical Non-radiative Accretion Flows in Two-Dimensions

390 citations · 1.5k across the 20 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2026

In-Situ Star Formation in a Thick Disk: A Model for Metal Enrichment of Mrk 573

Hannalore J. Gerling-Dunsmore, Mitchell C. Begelman, Jared A. Goldberg +2

Recent observations of the nearby Seyfert galaxy Mrk 573 found that the galactic nucleus and bicone regions surrounding the jet are significantly metal-enriched. In this paper, we…

astro-ph.HE2026

Electron-positron Pair Production in Global GRMHD Simulations of Black Hole Accretion Flows

Ho-Sang Chan, Jason Dexter, Mitchell C. Begelman

We present global, three-dimensional general relativistic magnetohydrodynamic simulations of accreting black holes that incorporate pair physics. Pairs are modeled as a passive sca…

astro-ph.HE2025

Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots

Matteo Cantiello, Jake B. Hassan, Rosalba Perna +5

The JWST discovery of "Little Red Dots" (LRDs) has revealed a population of compact, red sources at that likely host supermassive black holes (SMBHs). Recent observat…

astro-ph.HE2025★ 5 cited

Energy Diffusion and Advection Coefficients in Kinetic Simulations of Relativistic Plasma Turbulence

Kai W. Wong, Vladimir Zhdankin, Dmitri A. Uzdensky +2

Turbulent, relativistic nonthermal plasmas are ubiquitous in high-energy astrophysical systems, as inferred from broadband nonthermal emission spectra. The underlying turbulent non…

astro-ph.HE2012★ 104 cited

Three-dimensional AMR simulations of long-duration Gamma-Ray Burst jets inside massive progenitor stars

Diego López-Cámara, Brian J. Morsony, Micthell C. Begelman +1

We present the results of special relativistic, adaptive mesh refinement, 3D simulations of gamma-ray burst jets expanding inside a realistic stellar progenitor. Our simulations co…

astro-ph.HE2010★ 30 cited

X-ray flares from propagation instabilities in long Gamma-Ray Burst jets

Davide Lazzati, Chris H. Blackwell, Bran J. Morsony +1

We present a numerical simulation of a gamma-ray burst jet from a long-lasting engine in the core of a 16 solar mass Wolf-Rayet star. The engine is kept active for 6000 s with a lu…