activity
20162023
most citedEvidence of high-mass star formation through multi-scale mass accretion in hub-filament-system clouds

55 citations · 231 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202343 cited

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores

Shanghuo Li, Patricio Sanhueza, Qizhou Zhang +9

We present the dynamical properties of 294 cores embedded in twelve IRDCs observed as part of the ASHES Survey. Protostellar cores have higher gas masses, surface densities, column…

astro-ph.GA20235 cited

Deviation from a Continuous and Universal Turbulence Cascade in NGC 6334 due to Massive Star Formation Activity

Junhao Liu, Qizhou Zhang, Hauyu Baobab Liu +10

We use molecular line data from ALMA, SMA, JCMT, and NANTEN2 to study the multi-scale (15-0.005 pc) velocity statistics in the massive star formation region NGC 6334. We find…

astro-ph.GA202313 cited

Density Structure of Centrally Concentrated Prestellar Cores from Multi-scale Observations

Dipen Sahu, Sheng-Yuan Liu, Doug Johnstone +23

Starless cores represent the initial stage of evolution toward (proto)star formation, and a subset of them, known as prestellar cores, with high density (~ 10^6 cm^-3 or higher) an…

astro-ph.GA202355 cited

Evidence of high-mass star formation through multi-scale mass accretion in hub-filament-system clouds

Hong-Li Liu, Anandmayee Tej, Tie Liu +30

We present a statistical study of a sample of 17 hub-filament-system (HFS) clouds of high-mass star formation using high-angular resolution (1-2 arcsecond) ALMA 1.3mm and 3mm…

astro-ph.GA202230 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XII: Fragmentation and multi-scale gas kinematics in protoclusters G12.42+0.50 and G19.88-0.53

Anindya Saha, Anandmayee Tej, Hong-Li Liu +15

We present new continuum and molecular line data from the ALMA Three-millimeter Observations of Massive Star-forming regions (ATOMS) survey for the two protoclusters, G12.42+0.50 a…

astro-ph.GA20226 cited

Properties of dense molecular gas along the major axis of M 82

Fei Li, Zhi-Yu Zhang, Junzhi Wang +6

Dense gas is important for galaxy evolution and star formation. Optically-thin dense-gas tracers, such as isotopologues of HCN, HCO+, etc., are very helpful to diagnose excitation…