The magnetic field is a key ingredient in the recipe of star formation. However, the
importance of the magnetic field in the early stages of the formation of low-and high-mass …

The role of outflows in the formation of stars and the protostellar disks that generate them is
a central question in astrophysics. Outflows are associated with star formation across the …

Controlling and reversing the effects of loss are major challenges in optical systems. For
lasers, losses need to be overcome by a sufficient amount of gain to reach the lasing …

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 …

High-resolution Airborne Wide-band Camera (HAWC+) is the facility far-infrared imager and
polarimeter for SOFIA, NASA's Stratospheric Observatory for Infrared Astronomy. It is …

Although bipolar jets are seen emerging from a wide variety of astrophysical systems, the
issue of their formation and morphology beyond their launching is still under study. Our …

We present λ 1.3 mm Combined Array for Research in Millimeter-wave Astronomy
observations of dust polarization toward 30 star-forming cores and eight star-forming regions …

ABSTRACT Massive stars (M> 8 M☉) typically form in parsec-scale molecular clumps that
collapse and fragment, leading to the birth of a cluster of stellar objects. We investigate the …

We perform three-dimensional stratified shearing-box magnetohydrodynamic (MHD)
simulations on the gas dynamics of protoplanetary disks with a net vertical magnetic flux of B …

Context. Massive stars form in magnetized and turbulent environments and are often located
in stellar clusters. The accretion and outflows mechanisms associated with forming massive …