activity
20142026
most citedLocal Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak

160 citations · 619 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.HE2026

Geometrically Thin Sub-Eddington AGN Accretion Disks show a suppressed Lyman Edge

Ish Kaul, Yan-Fei Jiang, Omer Blaes +1

The observed ultraviolet continua of active galactic nuclei (AGN) generally lack a strong intrinsic HI Lyman edge predicted by classical optically thick accretion disk atmosphere m…

astro-ph.HE2026

Star-Disk Collisions II: Debris Stream Dynamics and Implications for QPEs and Other Transients Near SMBHs

Philippe Z. Yao, Eliot Quataert, Yan-Fei Jiang +1

Quasi-periodic eruptions (QPEs) are repeating soft X-ray nuclear transients with recurrence times of hours-days and flare duty cycles of 10-20%. Many aspects of QPEs can be m…

astro-ph.HE2026

PACHA: Probing AGN Coronae with High-redshift AGN

Xiurui Zhao, Elias Kammoun, Marco Ajello +18

The X-ray emission of active galactic nuclei (AGN) is generally attributed to inverse Compton scattering of accretion-disk photons by hot electrons in a compact corona. In local AG…

astro-ph.HE2026★ 1 cited

Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion

Lizhong Zhang, James M. Stone, Shane W. Davis +3

We present a comprehensive analysis of four near-Eddington black hole accretion models from GRMHD simulations with full radiation transport. This study investigates the dynamical e…

astro-ph.HE2025★ 1 cited

X-ray Variability and Photosphere Evolution during Accretion Disk Formation in Tidal Disruption Events

Xiaoshan Huang, Maria Renee Meza, Sol Bin Yun +3

The early time emission in tidal disruption events (TDEs) originates from both accretion and shocks, producing photons that eventually emerge from an inhomogeneous photosphere. We…

astro-ph.SR2025

Radiation Hydrodynamic Simulations of Low-Energy Explosions of Red and Yellow Supergiants

Andrea Antoni, Yan-Fei Jiang, Eliot Quataert

A variety of physical processes leads to the low-energy ejection of material from the hydrogen-rich envelopes of red and yellow supergiants. These include common envelope events, s…

astro-ph.HE2025

A Parameter Survey of Neutron Star Accretion Column Simulations

Lizhong Zhang, Omer Blaes, Yan-Fei Jiang

We conduct a parameter survey of neutron star accretion column simulations by solving the relativistic radiation MHD equations with opacities that account for strong magnetic field…

astro-ph.HE2025

Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks

Ish Kaul, Omer Blaes, Yan-Fei Jiang +1

Recent observations have revealed slow, coherent temperature fluctuations in AGN disks that propagate both inward and outward at velocities of , a kind of variabi…

astro-ph.HE2025

Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios

Lizhong Zhang, James M. Stone, Patrick D. Mullen +3

We summarize results from a survey of radiation-dominated black hole accretion flows across a wide range of mass accretion rates, as well as two values of black hole spin and initi…

astro-ph.HE2025

Radiation and Magnetic Pressure Support in Accretion Disks around Supermassive Black Holes and The Physical Origin of the Extreme Ultraviolet to Soft X-ray Spectrum

Yan-Fei Jiang, Omer Blaes, Ish Kaul +1

We present the results of four three-dimensional radiation magnetohydrodynamic simulations of accretion disks around a solar mass black hole, which produce the far ultraviol…

astro-ph.HE2025★ 4 cited

Non-Stationary Discs and Instabilities

Omer Blaes, Yan-Fei Jiang, Jean-Pierre Lasota +1

We review our current knowledge of thermal and viscous instabilities in accretion discs around compact objects. We begin with classical disc models based on analytic viscosity pres…

astro-ph.HE2024

Simulations of Eccentricity Growth in Compact Binary Accretion Disks with MHD Turbulence

Morgan Ohana, Yan-Fei Jiang, Omer Blaes +1

We present the results of four magnetohydrodynamic simulations and one alpha-disk simulation of accretion disks in a compact binary system, neglecting vertical stratification and a…

astro-ph.HE2024★ 1 cited

Numerical Simulations of Super-Eddington Accretion Flows

Yan-Fei Jiang, Lixin Dai

In this chapter, we summarize recent progress on the properties of accretion disks when the accretion rate exceeds the so-called Eddington limit based on multi-dimensional radiatio…

astro-ph.HE2024★ 1 cited

Star-Disk Collisions: Implications for Quasi-periodic Eruptions and Other Transients Near Supermassive Black Holes

Philippe Z. Yao, Eliot Quataert, Yan-Fei Jiang +2

We use Athena++ to study the hydrodynamics of repeated star-accretion disk collisions close to supermassive black holes, and discuss their implications for the origin of quasi-peri…

astro-ph.HE2024

Pre-peak Emission in Tidal Disruption Events

Xiaoshan Huang, Shane W. Davis, Yan-fei Jiang

The rising part of a tidal disruption event light curve provides unique insight into early emission and the onset of accretion. Various mechanisms are proposed to explain the pre-p…

astro-ph.HE2023

Reverberation evidence for Stream Collision and Delayed Disk Formation in Tidal Disruption Events

Hengxiao Guo, Jingbo Sun, Shuang-Liang Li +9

When a star passes through the tidal disruption radius of a massive black hole (BH), it can be torn apart by the tidal force of the BH, known as the Tidal Disruption Event (TDE). S…

astro-ph.HE2023★ 34 cited

An Extension of the Athena++ Code Framework for Radiation-Magnetohydrodynamics in General Relativity Using a Finite-Solid-Angle Discretization

Christopher J. White, Patrick D. Mullen, Yan-Fei Jiang +4

We extend the general-relativistic magnetohydrodynamics (GRMHD) capabilities of Athena++ to incorporate radiation. The intensity field in each finite-volume cell is discretized in…

astro-ph.HE2023★ 18 cited

A Bright First Day for Tidal Disruption Event

Xiaoshan Huang, Shane W. Davis, Yan-fei Jiang

Stream-stream collision may be an important pre-peak energy dissipation mechanism in tidal disruption events (TDEs). We perform local three-dimensional radiation hydrodynamic simul…

astro-ph.HE2023★ 26 cited

Global Three-Dimensional Radiation Magnetohydrodynamic Simulations of Accretion onto a Stellar Mass Black Hole at Sub- and Near-critical Accretion Rates

Jiahui Huang, Yan-Fei Jiang, Hua Feng +3

We present global 3D radiation magnetohydrodynamical simulations of accretion onto a 6.62 solar mass black hole with quasi-steady state accretion rates reaching 0.016 to 0.9 times…

astro-ph.GA2022★ 25 cited

CR Driven Multi-phase Gas Formed via Thermal Instability

Xiaoshan Huang, Yan-fei Jiang, Shane W. Davis

Cosmic rays (CRs) are an important energy source in the circum-galactic medium (CGM) that impact the multi-phase gas structure and dynamics. We perform two-dimensional CR-magnetohy…

astro-ph.HE2021★ 18 cited

Investigating lack of accretion disk eccentricity growth in a global 3D MHD simulation of a superhump system

Bryance Oyang, Yan-Fei Jiang, Omer Blaes

We present the results of a 3D global magnetohydrodynamic (MHD) simulation of an AM CVn system that was aimed at exploring eccentricity growth in the accretion disc self-consistent…

astro-ph.SR2016★ 19 cited

The Effects of Magnetic Fields on the Dynamics of Radiation Pressure Dominated Massive Star Envelopes

Yan-Fei Jiang, Matteo Cantiello, Lars Bildsten +2

We use three dimensional radiation magneto-hydrodynamic simulations to study the effects of magnetic fields on the energy transport and structure of radiation pressure dominated ma…

astro-ph.HE2016★ 153 cited

Prompt Radiation and Mass Outflows from the Stream-Stream Collisions of Tidal Disruption Events

Yan-Fei Jiang, James Guillochon, Abraham Loeb

Stream-stream collisions play an important role for the circularization of highly eccentric streams resulting from tidal disruption events (TDEs). We perform three dimensional radi…

astro-ph.HE2016★ 84 cited

Iron Opacity Bump Changes the Stability and Structure of Accretion Disks in Active Galactic Nuclei

Yan-Fei Jiang, Shane Davis, James Stone

Accretion disks around supermassive black holes have regions where the Rosseland mean opacity can be much larger than the electron scattering opacity primarily due to the large num…