Accretion through circumstellar disks plays an important role in star formation and in
establishing the properties of the regions in which planets form and migrate. The …

Recent spatially-resolved observations of protoplanetary disks revealed a plethora of
substructures, including concentric rings and gaps, inner cavities, misalignments, spiral …

The filamentary nature of accretion streams found around embedded sources suggests that
protostellar disks experience heterogenous infall from the star-forming environment …

The concentric gaps and rings commonly observed in protoplanetary disks in millimeter
continuum emission have lent the impression that planet formation generally proceeds …

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 …

High-mass protostars (M⋆> 8 M⊙) are thought to gain the majority of their mass via short,
intense bursts of growth. This episodic accretion is thought to be facilitated by gravitationally …

At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar
is deeply embedded in a dense, infalling envelope. We present the first systematic search …

DR Tau has been noted for its unusually high variability in comparison with other T Tauri
stars. Although it is one of the most extensively studied pre-main-sequence stars …

We investigate whether triggering of the magnetorotational instability (MRI) in protoplanetary
discs can account for the wide diversity of observed accretion outbursts. We show that short …