Observations of star-forming regions by the current and upcoming generation of
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …

Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey:
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …

The inner few hundred parsecs of the Milky Way harbours gas densities, pressures, velocity
dispersions, an interstellar radiation field and a cosmic ray ionization rate orders of …

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 …

Recent observations suggest an that intensive molecular cloud collision can trigger massive
star/cluster formation. The most important physical process caused by the collision is a …

In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

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

Observations indicate that molecular clouds are strongly magnetized, and that magnetic
fields influence the formation of stars. A key observation supporting the conclusion that …

We determine the magnetic field strength in the OMC 1 region of the Orion A filament via a
new implementation of the Chandrasekhar–Fermi method using observations performed as …