Star formation is a multi-scale, multi-physics problem ranging from the size scale of
molecular clouds (∼ 10 ∼10 s pc) down to the size scales of dense prestellar cores (∼ 0.1 …

In this review article, we aim at providing a global outlook on the progresses made in the
recent years to characterize the role of magnetic fields during the embedded phases of the …

Context. Studies of Class 0 objects allow to characterize the dynamical processes taking
place at the onset of the star formation process and to determine the physical mechanisms …

We present and release the full data set for the Mass Assembly of Stellar Systems and their
Evolution with the SMA (MASSES) survey. This survey used the Submillimeter Array (SMA) …

We present ALMA 3 mm molecular line and continuum observations with a resolution of∼
3.5 arcsec towards five first hydrostatic core (FHSC) candidates (L1451-mm, Per-bolo 58 …

We present the results on the physical properties of filaments and dense cores in IC 5146,
as a part of the TRAO FUNS project. We carried out on-the-fly mapping observations using …

We report ALMA Cycle 3 observations in CO isotopes toward a dense core, MC27/L1521F in
Taurus, which is considered to be at an early stage of multiple star formation in a turbulent …

Context. The formation of stars has been subject to extensive studies in the past decades on
scales from molecular clouds to proto-planetary disks. It is still not fully understood how the …

We present our current understanding of the formation and early evolution of protostars,
protoplanetary disks, and the driving of outflows as dictated by the interplay of magnetic …

Abstract" TRAO FUNS" is a project to survey the Gould Belt's clouds in molecular lines. This
paper presents its first results on the central region of the California molecular cloud, L1478 …