We present an overview of the Large Program," Early Planet Formation in Embedded Disks
(eDisk)," conducted with the Atacama Large Millimeter/submillimeter Array (ALMA). The …

▪ Abstract The physical conditions in molecular clouds control the nature and rate of star
formation, with consequences for planet formation and galaxy evolution. The focus of this …

We carry out radiation hydrodynamic calculations to study physical processes in the
formation of a 1 M⊙ protostar. Following our previous work, calculations pursue the whole …

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 …

We present ALMA 1.3 mm continuum, 12 CO, C 18 O, and SO data for the Class 0 protostars
Lupus 3 MMS, IRAS 15398− 3559, and IRAS 16253− 2429 at resolutions of∼ 100 au. By …

We present multiline and continuum observations of the circumstellar environment within 10
4 AU of a sample of protostars to investigate how the effects of outflows on their immediate …

We have observed the Class I protostar TMC-1A with the Atacama Millimeter/submillimeter
Array (ALMA) in the emissions of 12 CO and C 18 O (J= 2–1) and 1.3 mm dust continuum …

We have conducted ALMA observations in the 1.3 mm continuum and 12 CO (2–1), C 18 O
(2–1), and SO (5 6–4 5) lines toward L1489 IRS, a Class I protostar surrounded by a …

We present the results of an imaging survey of protoplanetary disks around single T Tauri
stars in Taurus. Thermal emission at 2 mm from dust in the disks has been imaged with a …

Context. Disks are observed around pre-main sequence stars, but how and when they form
is still heavily debated. While disks around young stellar objects have been identified …