activity
20242026
collaborators

11 papers

astro-ph.CO2026

High Resolution Grid-based Simulations of the Warm-Hot Intergalactic Medium

Lile Wang, Renyue Cen

We present high-resolution cosmological hydrodynamic simulations of the Warm-Hot Intergalactic Medium (WHIM) using the GPU-optimized grid-based hydrodynamic code Kratos. Employing…

astro-ph.HE2026

From Inspiral to Expansion: The Wake-Driven Torque on Binary Black Holes in Gaseous Medium

Jixuan Yang, Lile Wang, Xinyu Li +1

Binary black holes (BBHs) in gaseous medium, such as active galactic nucleus (AGN) disks, are important gravitational-wave sources, yet the gas-driven torque that governs their orb…

astro-ph.GA2026

HOTDISK. Finding Massive Protostellar Disks with Water and Refractory Molecular Species

Kai Yang, Yichen Zhang, Kei E. I. Tanaka +16

We present high-angular-resolution (, au) ALMA Band~6 observations from the HOTDISK project (Hot-Origin Tracer survey of DISKs of massive pro…

astro-ph.GA2026

The effects of star-gas interactions on binary evolution in open clusters

Jixuan Yang, Lile Wang, Xinyu Li +3

Star-gas interactions can provide gravitational feedback that influences the dynamical evolution of stellar clusters, through processes such as dynamical friction (DF) and its non-…

astro-ph.EP2025

Consistent Modeling of Non-equilibrium Dust Sublimation and the Interactions with Dust Evolution in the Inner Regions of Protoplanetary Disks

Sheng Xu, Lile Wang, Luis C. Ho +2

The inner regions of protoplanetary disks are host to the sublimation of dust grains, a process traditionally modeled using equilibrium thermodynamics. We demonstrate through ab-in…

astro-ph.GA2025

AGN star dynamics under the Influence of Outflow-Ambient Interactions

Muxin Liu, Lile Wang, Peng Peng

Stars with outflows interacting with ambient gas experience accelerations arising from the gravitational feedback induced by the interaction structure. In this work, three-dimensio…

astro-ph.GA2025

Disturbed cold gas in galaxy and structure formation

Siwei Zou, Robert A. Simcoe, Patrick Petitjean +18

Cold and cool gas (T K) in the circumgalactic medium (CGM) and its interaction with galaxies remain poorly understood. Simulations predict that cold gas flows into gala…

astro-ph.GA2024

Turbulent Diffuse Molecular Media with Non-ideal Magnetohydrodynamics and Consistent Thermochemistry: Numerical Simulations and Dynamic Characteristics

Nannan Yue, Lile Wang, Thomas Bisbas +2

Turbulent diffuse molecular clouds can exhibit complicated morphologies caused by the interactions among radiation, chemistry, fluids, and fields. We performed full 3D simulations…

astro-ph.GA2024

Cloud Crushing and Dissipation of Uniformly-Driven Adiabatic Turbulence in Circumgalactic Media

Alex Lv, Lile Wang, Renyue Cen +1

The circumgalactic medium (CGM) is responsive to kinetic disruptions generated by nearby astrophysical events. In this work, we study the saturation and dissipation of turbulent hy…

astro-ph.GA2024

FEASTS Combined with Interferometry (I): Overall Properties of Diffuse HI and Implications for Gas Accretion in Nearby Galaxies

Jing Wang, Xuchen Lin, Dong Yang +19

We present a statistical study of the properties of diffuse HI in ten nearby galaxies, comparing the HI detected by the single-dish telescope FAST (FEASTS program) and the interfer…

astro-ph.GA2024

Open Cluster Dynamics under the Influence of Outflow-Ambient Interactions

Muxin Liu, Lile Wang, Xiaoting Fu +1

Stars with outflows impinging on ambient gas experience accelerations due to the gravitational feedback from the interaction morphology between the outflow and the ambient gas. Suc…