We present observations of the Class 0 protostar IRAS 16544–1604 in CB 68 from the" Early
Planet Formation in Embedded Disks (eDisk)" ALMA Large program. The ALMA …

The origin of complex organic molecules (COMs) in young Class 0 protostars has been one
of the major questions in astrochemistry and star formation. While COMs are thought to form …

Protostellar disks are an ubiquitous part of the star formation process and the future sites of
planet formation. As part of the Early Planet Formation in Embedded Disks large program …

We report on an Atacama Large Millimeter/submillimeter Array study of the Class I or II
intermediate-mass protostar DK Cha in the Chamaeleon II region. The 12 CO (J= 2–1) …

We present the detection of a secondary outflow associated with a Class I source, Ser-emb
15, in the Serpens Molecular Cloud. We reveal two pairs of molecular outflows consisting of …

We present the four-year survey results of monthly submillimeter monitoring of eight nearby
(< 500 pc) star-forming regions by the JCMT Transient Survey. We apply the Lomb–Scargle …

Abstract Brown Dwarfs (BDs) are crucial objects in our understanding of both star and planet
formation, as well as in our understanding of what mechanisms shape the lower end of the …

The huge variety of planetary systems discovered in recent decades likely depends on the
early history of their formation. In this contribution, we introduce the FAUST Large Program …

The angular momentum of molecular cloud cores plays an important role in the process of
star formation. However, the time evolution of the angular momentum of molecular cloud …

Observed changes in protostellar brightness can be complicated to interpret. In our James
Clerk Maxwell Telescope (JCMT) Transient Monitoring Survey, we discovered that a young …