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20152026
most citedSimulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies

65 citations · 206 across the 12 of their papers we have counts for

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Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2026

A Nonlinear General Implicit Runge-Kutta Integrator for Multifluid Charged Dust and Gas

Mengxuan Chen, Hui Li, Chong-Chong He +3

Charged dust in magnetized gas is subject to aerodynamic drag and the Lorentz force, both of which can be difficult to model numerically in a fluid simulation where their character…

astro-ph.GA2024★ 2 cited

A novel numerical method for mixed-frame multigroup radiation-hydrodynamics with GPU acceleration implemented in the QUOKKA code

Chong-Chong He, Benjamin D. Wibking, Mark R. Krumholz

Mixed-frame formulations of radiation-hydrodynamics (RHD), where the radiation quantities are computed in an inertial frame but matter quantities are in a comoving frame, are advan…

astro-ph.GA2024★ 1 cited

Formation of Large Circumstellar Discs in Multi-scale, ideal-MHD Simulations of Magnetically Critical Pre-stellar Cores

Chong-Chong He, Massimo Ricotti

The formation of circumstellar discs is a critical step in the formation of stars and planets. Magnetic fields can strongly affect the evolution of angular momentum during prestell…

astro-ph.GA2022★ 5 cited

Bimodal Star Formation in Simulations of Strongly Magnetized Giant Molecular Clouds

Ronan Hix, Chong-Chong He, Massimo Ricotti

We present the results of a set of radiation magnetohydrodynamic simulations of turbulent molecular clouds in which we vary the initial strength of the magnetic field within a rang…

astro-ph.GA2022★ 11 cited

Massive Prestellar Cores in Radiation-magneto-turbulent Simulations of Molecular Clouds

Chong-Chong He, Massimo Ricotti

We simulate the formation and collapse of prestellar cores at few-AU resolution in a set of radiation-magneto-hydrodynamic simulations of giant molecular clouds (GMCs) using the gr…

astro-ph.GA2021★ 6 cited

A Fast and Accurate Analytic Method of Calculating Galaxy Two-point Correlation Functions

Chong-Chong He

We have developed a new analytic method to calculate the galaxy two-point correlation functions (TPCFs) accurately and efficiently, applicable to surveys with finite, regular, and…

astro-ph.GA2020★ 38 cited

Simulating Star Clusters Across Cosmic Time: II. Escape Fraction of Ionizing Photons from Molecular Clouds

Chong-Chong He, Massimo Ricotti, Sam Geen

We calculate the hydrogen and helium-ionizing radiation escaping star-forming molecular clouds, as a function of the star cluster mass and compactness, using a set of high-resoluti…

astro-ph.GA2019★ 65 cited

Simulating Star Clusters Across Cosmic Time: I. Initial Mass Function, Star Formation Rates and Efficiencies

Chong-Chong He, Massimo Ricotti, Sam Geen

We present radiation-magneto-hydrodynamic simulations of star formation in self-gravitating, turbulent molecular clouds, modeling the formation of individual massive stars, includi…