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20212025
most citedNumerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes

72 citations · 241 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025

Type IIb Supernova Progenitors in 3D: Variability and Episodic Mass Loss revealed by Radiation-Hydrodynamics Simulations

Jared A. Goldberg, Yan-Fei Jiang, Lars Bildsten +1

We present the first 3D Radiation-Hydrodynamics simulations of partially-stripped (, ) Yellow Supergiant (,…

astro-ph.HE2024★ 1 cited

Local models of two-temperature accretion disc coronae. II. Ion thermal conduction and the absence of disc evaporation

Christopher J. Bambic, Eliot Quataert, Matthew W. Kunz +1

We use local stratified shearing-box simulations with magnetic field-aligned thermal conduction to study an idealized model of the coupling between a cold, radiatively efficient ac…

astro-ph.GA2023★ 26 cited

A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation

Sophie Koudmani, Rachel S. Somerville, Debora Sijacki +3

It is well established that supermassive black hole (SMBH) feedback is crucial for regulating the evolution of massive, if not all, galaxies. However, modelling the interplay betwe…

astro-ph.SR2023★ 13 cited

Three Dimensional Natures of Massive Star Envelopes

Yan-Fei Jiang

We review our current understanding on the outer envelope structures of massive stars based on three dimensional (3D) radiation hydrodynamic simulations. We briefly summarize the f…

astro-ph.SR2023★ 16 cited

Turbulence Supported Massive Star Envelopes

William Schultz, Lars Bildsten, Yan-Fei Jiang

The outer envelopes of massive () stars exhibit large increases in opacities from forests of lines and ionization transitions (particularly from iron and hel…

astro-ph.SR2022★ 13 cited

Synthesizing Spectra from 3D Radiation Hydrodynamic Models of Massive Stars Using Monte Carlo Radiation Transport

William C. Schultz, Benny T. H. Tsang, Lars Bildsten +1

Observations indicate that turbulent motions are present on most massive star surfaces. Starting from the observed phenomena of spectral lines with widths much larger than thermal…

astro-ph.SR2022★ 58 cited

Shock Breakout in 3-Dimensional Red Supergiant Envelopes

Jared A. Goldberg, Yan-fei Jiang, Lars Bildsten

Using Athena++, we perform 3D Radiation-Hydrodynamic calculations of the radiative breakout of the shock wave in the outer envelope of a red supergiant (RSG) which has suffered cor…

astro-ph.SR2021★ 42 cited

Stochastic Low Frequency Variability in 3-Dimensional Radiation Hydrodynamical Models of Massive Star Envelopes

William C. Schultz, Lars Bildsten, Yan-Fei Jiang

Increasing main sequence stellar luminosity with stellar mass leads to the eventual dominance of radiation pressure in stellar envelope hydrostatic balance. As the luminosity appro…

astro-ph.SR2021★ 72 cited

Numerical Simulations of Convective 3-Dimensional Red Supergiant Envelopes

Jared A. Goldberg, Yan-Fei Jiang, Lars Bildsten

We explore the three-dimensional properties of convective, luminous (), Hydrogen-rich envelopes of Red Supergiants (RSGs) based on radiation hydrody…