While dust disks around optically visible, Class II protostars are found to be vertically thin,
when and how dust settles to the midplane are unclear. As part of the Atacama Large …

Precise estimates of protostellar masses are crucial to characterize the formation of stars of
low masses down to brown dwarfs (BDs; M*< 0.08 M☉). The most accurate estimation of …

The envelopes and disks that surround protostars reflect the initial conditions of star and
planet formation and govern the assembly of stellar masses. Characterizing these structures …

The mantra “know thy star, know thy planet” has proven to be very important for many
aspects of exoplanet science. Here I review how stellar abundances inform our …

Constraining the physical and chemical structure of young embedded disks is crucial for
understanding the earliest stages of planet formation. As part of the Early Planet Formation …

We have observed the Class 0/I protostellar system Ced110 IRS4 at an angular resolution of
0 farcs 05 (∼ 10 au) as part of the Atacama Large Millimeter/submillimeter Array large …

Studying the physical and chemical conditions of young embedded disks is crucial to
constrain the initial conditions for planet formation. Here we present Atacama Large …

Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of
the Class I source Oph IRS 63 in the context of the Early Planet Formation in Embedded …

Characterizing the physical properties of dust grains in a protoplanetary disk is critical to
comprehending the planet formation process. Our study presents Atacama Large Millimeter …

Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion
phase and encode the history of stellar accretion, complex organic molecule (COM) …