We present results from the first population synthesis study of protostellar discs. We analyse
the evolution and properties of a large sample of protostellar discs formed in a radiation …

Context. Understanding the formation mechanisms of protoplanetary disks and multiple
systems and also their pristine properties are key questions for modern astrophysics. The …

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 …

HH 212 is a nearby (400 pc) Class 0 protostellar system recently found to host a"
hamburger"-shaped dusty disk with a radius of∼ 60 au, deeply embedded in an infalling …

With the aim of characterizing the dynamical processes involved in the formation of young
protostars, we present highangular-resolution ALMA dust polarization observations of the …

The formation of protoplanetary disks is not well understood. To understand how and when
these disks are formed, it is crucial to characterize the kinematics of the youngest protostars …

HH 211-mms is one of the youngest Class 0 protostellar systems in Perseus, at a distance
of∼ 235 pc. We have mapped its central region at up to∼ 7 au (0 farcs 03) resolution. A …

ALMA Observations of the Protostar L1527 IRS: Probing Details of the Disk and the Envelope
Structures - IOPscience This site uses cookies. By continuing to use this site you agree to our …

Polarized emission is detected in two young nearly edge-on protostellar disks in 343 GHz
continuum at∼ 50 au (∼ 0 farcs 12) resolution with Atacama Large Millimeter/submillimeter …

We compare the directions of molecular outflows of 62 low-mass Class 0 and I protostars in
nearby (< 450 pc) star-forming regions with the mean orientations of the magnetic fields on …