activity
20012024
most citedSimulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP

318 citations · 2.1k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2024

The ALMA-QUARKS Survey: Fibers' role in star formation unveiled in an intermediate-mass protocluster region of the Vela D cloud

Dongting Yang, HongLi Liu, Tie Liu +32

In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of ), using ALMA data fro…

astro-ph.GA2024

The ALMA-QUARKS survey: Detection of two extremely dense substructures in a massive prestellar core

Xiaofeng Mai, Tie Liu, Xunchuan Liu +32

Only a handful of massive starless core candidates have been discovered so far, but none of them have been fully confirmed. Within the MM1 clump in the filamentary infrared dark cl…

astro-ph.GA2022★ 86 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XI. From inflow to infall in hub-filament systems

Jian-Wen Zhou, Tie Liu, Neal J. Evans +37

We investigate the presence of hub-filament systems in a large sample of 146 active proto-clusters, using HCO J=1-0 molecular line data obtained from the ATOMS survey.…

astro-ph.GA2022★ 11 cited

The Role of Magnetic Fields in the Stability and Fragmentation of Filamentary Molecular Clouds: Two Case Studies at OMC-3 and OMC-4

Pak Shing Li, Enrique Lopez-Rodriguez, Archana Soam +1

We present the stability analysis of two regions, OMC-3 and OMC-4, in the massive and long molecular cloud complex of Orion A. We obtained m HAWC+/SOFIA polarization data, a…

astro-ph.GA2022★ 25 cited

The Davis-Chandrasekhar-Fermi Method Revisited

Che-Yu Chen, Zhi-Yun Li, Renato R. Mazzei +5

Despite the rich observational results on interstellar magnetic fields in star-forming regions, it is still unclear how dynamically significant the magnetic fields are at varying p…

astro-ph.GA2022★ 13 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): How do dense core properties affect the multiplicity of protostars?

Qiuyi Luo, Tie Liu, Kenichi Tatematsu +34

During the transition phase from a prestellar to a protostellar cloud core, one or several protostars can form within a single gas core. The detailed physical processes of this tra…