Molecular clouds are a fundamental ingredient of galaxies: they are the channels that
transform the diffuse gas into stars. The detailed process of how they do it is not completely …

We present and discuss the results of the Herschel Gould Belt survey (HGBS) observations
in an~ 11 deg 2 area of the Aquila molecular cloud complex at d~ 260 pc, imaged with the …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …

Context. Molecular filaments have received special attention recently thanks to new
observational results on their properties. In particular, our early analysis of filament …

Star formation is primarily controlled by the interplay between gravity, turbulence, and
magnetic fields. However, the turbulence and magnetic fields in molecular clouds near the …

Filaments are ubiquitous in the Universe. Recent observations have revealed that stars and
star clusters form preferentially along dense filaments. Understanding the formation and …

We present the Planck Catalogue of Galactic Cold Clumps (PGCC), an all-sky catalogue of
Galactic cold clump candidates detected by Planck. This catalogue is the full version of the …

We use a suite of high-resolution molecular cloud simulations carried out with the moving
mesh code arepo to explore the nature of star-forming filaments. The simulated filaments are …

The ubiquity of filamentary structure at various scales throughout the Galaxy has triggered a
renewed interest in their formation, evolution, and role in star formation. The largest …

The ATOMS, standing for ALMA Three-millimeter Observations of Massive Star-forming
regions, survey has observed 146 active star-forming regions with ALMA band 3, aiming to …