Star cluster progenitors are dynamically decoupled from their parent molecular clouds

N Peretto, AJ Rigby, F Louvet, GA Fuller… - Monthly Notices of …, 2023 - academic.oup.com
The formation of stellar clusters dictates the pace at which galaxies evolve, and solving the
question of their formation will undoubtedly lead to a better understanding of the Universe as …

WISDOM Project–XII. Clump properties and turbulence regulated by clump–clump collisions in the dwarf galaxy NGC 404

L Liu, M Bureau, GX Li, TA Davis… - Monthly Notices of …, 2022 - academic.oup.com
We present a study of molecular structures (clumps and clouds) in the dwarf galaxy NGC
404 using high-resolution (≈ 0.86× 0.51 pc2) Atacama Large Millimeter/sub-millimeter Array …

Physical and chemical structure of the Serpens filament: Fast formation and gravity-driven accretion

Y Gong, A Belloche, FJ Du, KM Menten… - Astronomy & …, 2021 - aanda.org
Context. The Serpens filament, a prominent elongated structure in a relatively nearby
molecular cloud, is believed to be at an early evolutionary stage, so studying its physical and …

Scale-free gravitational collapse as the origin of ρ ∼ r−2 density profile – a possible role of turbulence in regulating gravitational collapse

GX Li - Monthly Notices of the Royal Astronomical Society, 2018 - academic.oup.com
Astrophysical systems, such as clumps that form star clusters share a density profile that is
close to ρ∼ r− 2. We prove analytically this density profile is the result of the scale-free …

Effective shielding of≲ 10 GeV cosmic rays from dense molecular clumps

R Yang, GX Li, EO Wilhelmi, YD Cui, B Liu… - Nature …, 2023 - nature.com
The density of cosmic rays inside molecular clouds determines the ionization rate in the
dense cores where stars form. It is also one of the drivers of astrochemistry leading to the …

Morphology of molecular clouds at kiloparsec scale in the Milky Way: Shear-induced alignment and vertical confinement

YH Xie, GX Li, BQ Chen - The Astrophysical Journal, 2024 - iopscience.iop.org
The shape of the cold interstellar molecular gas is determined by several processes,
including self-gravity, tidal force, turbulence, magnetic field, and galactic shear. Based on …

Jeans instability and turbulent gravitational collapse of Bose–Einstein condensate dark matter halos

T Harko - The European Physical Journal C, 2019 - Springer
We consider the Jeans instability and the gravitational collapse of the rotating Bose–Einstein
condensate dark matter halos, described by the zero temperature non-relativistic Gross …

Magnetic Fields in Giant Filaments Probed by the Velocity Gradient Technique: Regular Magnetic Field Interrupted by Magnetization Gaps

M Zhao, GX Li, J Zhou, X Tang, J Esimbek… - The Astrophysical …, 2024 - iopscience.iop.org
We study the magnetic field structures in six giant filaments associated with the spiral arms
of the Milky Way by applying the velocity gradient technique (VGT) to the 13 CO …

Mass–size scaling M ∼ r1.67 of massive star-forming clumps – evidences of turbulence-regulated gravitational collapse

CP Zhang, GX Li - Monthly Notices of the Royal Astronomical …, 2017 - academic.oup.com
We study the fragmentation of eight massive clumps using data from ATLASGAL 870 μm,
SCUBA 850 and 450 μm, PdBI 1.3 and 3.5 mm, and probe the fragmentation from 1 to 0.01 …

The ALMA-QUARKS Survey. II. The ACA 1.3 mm Continuum Source Catalog and the Assembly of Dense Gas in Massive Star-Forming Clumps

F Xu, K Wang, T Liu, L Zhu, G Garay… - … in Astronomy and …, 2024 - iopscience.iop.org
Leveraging the high resolution, sensitivity, and wide frequency coverage of the Atacama
Large Millimeter/submillimeter Array (ALMA), the QUARKS survey, standing for" Querying …