activity
20242026
collaborators

15 papers

astro-ph.GA2026

Morphological Identification of Dynamical Regimes in MHD Turbulence with ScaleAware-JEPA

Mengke Zhao, Guang-Xing Li, Keping Qiu

The morphology of turbulent interstellar gas reflects the coupled action of turbulence, magnetic fields, and self-gravity, but density amplitude alone does not uniquely specify dyn…

astro-ph.GA2026

Gravity-driven Emergence of Multi-fractal Density Structure in the Orion A Integral Shaped Filament

Mengke Zhao, Guang-Xing Li, Keping Qiu +1

Molecular clouds are often described as self-similar structures, although spatially averaged measures do not retain local variations in density scaling. We use the density exponent…

astro-ph.IM2026

Scale-Vector Alignment: A Scale-Aware Framework for Spatially Resolved Morphological Similarity in Astronomical Images

Mengke Zhao, Guang-Xing Li, Keping Qiu +1

Astronomical maps made with different tracers are not expected to have identical morphology. Excitation, optical depth, chemistry, radiation, and ISM phase alter the response of a…

astro-ph.GA2026

Turbulence Cascade in Cygnus X Revealed by Multi-point VDF Method

Junjie Huang, Yangjun Pu, Keping Qiu +3

Turbulence plays a crucial role in regulating star formation activities within molecular clouds, yet few methods can directly reveal its properties and underlying processes. We use…

astro-ph.GA2026

A Unified Magnetohydrodynamic Scaling Relation for the Multiphase Interstellar Medium

Mengke Zhao, Guang-Xing Li, Keping Qiu

The interplay of magnetic fields, turbulence, and gravity governs the structural evolution of the interstellar medium (ISM) and the initial conditions of star formation, yet observ…

astro-ph.GA2026

BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW

Mengke Zhao, Keping Qiu, Ji-hyun Kang +27

We present high-resolution magnetic field maps of the M17 SW molecular cloud using JCMT 850 m dust polarization at a scale of 14. The magnetic field exhibits a distinct arc-…

cs.LG2026

Scale-Aware Adversarial Analysis: A Diagnostic for Generative AI in Multiscale Complex Systems

Mengke Zhao, Guang-Xing Li, Duo Xu +1

Complex physical systems, from supersonic turbulence to the macroscopic structure of the universe, are governed by continuous multiscale dynamics. While modern machine learning arc…

astro-ph.GA2026

ALMA Polarization Study of the Magnetic Fields in Two Massive Clumps in the 20 km s Cloud of the Central Molecular Zone

Yuhua Liu, Xing Lu, Junhao Liu +14

We present the Atacama Large Millimeter/submillimeter Array (ALMA) observations of linearly polarized 870 m continuum emission at a resolution of 0.2 (200…

astro-ph.GA2025

Galactic Contrail in NGC 3627 caused by Dwarf Galaxy Candidate or Massive Black Hole Flyby

Mengke Zhao, Guang-Xing Li

We report the discovery of a kpc scale molecular contrail in the spiral galaxy NGC 3627, a narrow structure spanning 8 kpc in length with a width of 200 pc and an extreme aspect ra…

astro-ph.IM2025

Volume Density Mapper: 3D Density Reconstruction Algorithm for Molecular Clouds

Guang-Xing Li, Mengke Zhao

The interstellar medium (ISM) exhibits complex, multi-scale structures that are challenging to study due to their projection into two-dimensional (2D) column density maps. We prese…

astro-ph.GA2025

Equation vs. AI: Predict Density and Measure Width of molecular clouds by Multiscale Decomposition

Mengke Zhao, Guang-Xing Li, Duo Xu +1

Interstellar medium widely exists in the universe at multi-scales. In this study, we introduce the {\it Multi-scale Decomposition Reconstruction} method, an equation-based model de…

astro-ph.GA2024

Super-Jeans fragmentation in massive star-forming regions revealed by triangulation analysis

Guang-Xing Li, Mengke Zhao, Xing Lu

Understanding the fragmentation of the gas cloud and the formation of massive stars remains one of the most challenging questions of modern astrophysical research. Either the gas f…

astro-ph.GA2024

Slope of Magnetic Field-Density Relation as An Indicator of Magnetic Dominance

Mengke Zhao, Guang-Xing Li, Keping Qiu

The electromagnetic field is a fundamental force in nature that regulates the formation of stars in the universe. Despite decades of efforts, a reliable assessment of the importanc…

astro-ph.GA2024

Magnetic, Kinetic, and Transition Regime: Spatially-Segregated Structure of Compressive MHD Turbulence

Guang-Xing Li, Mengke Zhao

Turbulence is a complex physical process prevalent in modern physics, particularly in ionized environments like interstellar gas, where magnetic fields play a dynamic role. However…

astro-ph.GA2024

Curvature Mapping Method: Mapping Lorentz Force in Orion A

Mengke Zhao, Guang-Xing Li, Keping Qiu

Magnetic force is a fundamental force in nature. Although widely believed to be important in counterbalancing against collapse in star formation, a clear evaluation of the role of…