Aim. We have investigated the gas organization within the paradigmatic Integral Shape
Filament (ISF) in Orion in order to decipher whether or not all filaments are bundles of fibers …

We investigate the presence of hub-filament systems in a large sample of 146 active proto-
clusters, using H13CO+ J= 1-0 molecular line data obtained from the ATOMS survey. We …

Filamentary structures are ubiquitous in high-mass star-forming molecular clouds. Their
relation with high-mass star formation is still to be understood. Here we report interferometric …

Context. Converging networks of interstellar filaments, that is hubs, have been recently
linked to the formation of stellar clusters and massive stars. Understanding the relationship …

Context. Dense molecular filaments are ubiquituous in the interstellar medium, yet their
internal physical conditions and the role of gravity, turbulence, the magnetic field, radiation …

We study the fragmentation of the nearest high line-mass filament, the integral shaped
filament (ISF, line-mass~ 400 M⊙ pc-1) in the Orion A molecular cloud. We have observed a …

The surroundings of massive protostars constitute an accretion disc which has numerically
been shown to be subject to fragmentation and responsible for luminous accretion-driven …

In typical environments of star-forming clouds, converging supersonic turbulence generates
shock-compressed regions, and can create strongly magnetized sheet-like layers …

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 …

Young stellar populations provide a record of past star formation, and by establishing their
members' dynamics and ages, it is possible to reconstruct the full history of star formation …