Context. Cygnus X is one of the closest and most active high-mass star-forming regions in
our Galaxy, making it one of the best laboratories for studying massive star formation. Aims …

We present 850 μm dust polarization observations of the massive DR21 filament from the B-
fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter …

We studied the hub-filament system G323. 46-0.08 based on archival molecular line data
from the SEDIGISM 13 CO survey and infrared data from the GLIMPSE, MIPS, and Hi-GAL …

We present deep, sub-arcsecond (2000 au) resolution ALMA 0.82-mm observations of the
former high-mass prestellar core candidate G11. 92–0.61 MM2, recently shown to be an 500 …

Abstract DR21 (OH) ridge, the central part of a high-mass star-and cluster-forming hub-
filament system, is resolved spatially and kinematically into three nearly parallel fibers (f1, f2 …

Using the H i self-absorption data from the Five-hundred-meter Aperture Spherical radio
Telescope, we perform a study of the cold atomic gas in the Cygnus X North region. The …

Filamentary structures are closely associated with star-forming cores, but their detailed
physical connections are still not clear. We studied the dense gas in OMC-3 MMS-7 region …

Filamentary flows towards the centre of molecular clouds have been recognized as a crucial
process in the formation and evolution of stellar clusters. In this paper, we present a …

We present one of the first Shanghai Tian Ma Radio Telescope (TMRT) K Band observations
towards a sample of 26 infrared dark clouds (IRDCs). We observed the (1, 1),(2, 2),(3, 3) …

Context. Identified as parsec-size, gas clumps at the junction of multiple filaments, hub-
filament systems (HFS) play a crucial role during the formation of young clusters and high …