activity
20172026
most citedA holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields

81 citations · 525 across the 31 of their papers we have counts for

collaborators
Showing 2023Show all

5 papers · 1 filter

astro-ph.GA2023

ALMA High-resolution Spectral Survey of Thioformaldehyde (H2CS) Towards Massive Protoclusters

Li Chen, Sheng-Li Qin, Tie Liu +12

Investigating the temperature and density structures of gas in massive protoclusters is crucial for understanding the chemical properties therein. In this study, we present observa…

astro-ph.GA2023

A low-mass line-rich core found in Massive Star-forming Region IRAS 16351-4722

Meizhu Liu, Sheng-Li Qin, Tie Liu +10

We present ALMA sub-arcsecond-resolution observations of both continuum and molecular lines at 345 GHz towards the massive star-forming region IRAS 16351-4722 (hereafter I16351). A…

astro-ph.GA2023★ 1 cited

The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE): Core Growth, Cluster Contraction, and Primordial Mass Segregation

Fengwei Xu, Ke Wang, Tie Liu +40

The ALMA Survey of Star Formation and Evolution in Massive Protoclusters with Blue Profiles (ASSEMBLE) aims to investigate the process of mass assembly and its connection to high-m…

astro-ph.GA2023

An initial analysis of a strongly-lensed QSOs candidate identified by LAMOST

Y. H. Chen, M. Y. Tang, H. Shu +1

From 2011 to 2021, LAMOST has released a total of 76,167 quasar data. We try to search for gravitationally lensed QSOs by limiting coordinate differences and redshift differences o…

astro-ph.GA2023★ 71 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335

Feng-Wei Xu, Ke Wang, Tie Liu +37

We present ALMA Band-3/7 observations towards "the Heart" of a massive hub-filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a resolution of $\sim0.0…