Star-forming regions show a rich and varied chemistry, including the presence of complex
organic molecules—in both the cold gas distributed on large scales and the hot regions …

We review recent advances in our understanding of magnetism in the solar nebula and
protoplanetary disks (PPDs). We discuss the implications of theory, meteorite …

Context. In the past few years, there has been a rise in the detection of streamers,
asymmetric flows of material directed toward the protostellar disk with material from outside …

Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

Variability in young stellar objects (YSOs) can be caused by various time-dependent
phenomena associated with star formation, including accretion rates, geometric changes in …

We present the latest development of the disk gravitational instability and fragmentation
model, originally introduced by us to explain episodic accretion bursts in the early stages of …

Based on sub-arcsecond Atacama Large Millimeter/submillimeter Array (ALMA) and
Submillimeter Array (SMA) 1.3 mm continuum images of the massive protocluster NGC …

We have conducted a homogeneous near-infrared (near-IR) spectroscopic survey of 33
objects with varying degrees of similarity to FU Orionis. Common spectroscopic features that …

Complex organic molecules (COMs), which are the seeds of prebiotic material and
precursors of amino acids and sugars, form in the icy mantles of circumstellar dust grains but …