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 …

Context. Recent observations suggest that planet formation starts early, in protostellar disks
of≤ 10 5 yr, which are characterized by strong interactions with the environment, such as …

Context. Elongated trails of infalling gas, often referred to as “streamers,” have recently been
observed around young stellar objects (YSOs) at different evolutionary stages. This …

Transferring a significant fraction of the magnetic flux from a dense cloud core is essential in
the star formation process. A ringlike structure produced by magnetic flux loss has been …

The ALMA interferometer has played a key role in revealing a new component of the Sun-
like star forming process: the molecular streamers, ie structures up to thousands of au long …

High-resolution, millimeter observations of disks at the protoplanetary stage reveal
substructures such as gaps, rings, arcs, spirals, and cavities. While many protoplanetary …

We present ALMA Band 7 molecular line observations of the protostars within the VLA 1623
system. We detect C 17 O (3–2) in the circumbinary disk around VLA 1623A and the outflow …

Abstract Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations have
revealed an increasing number of compact protostellar disks with radii of less than a few …

To investigate the formation process of multiple systems, we have analyzed the Atacama
Large Millimeter/submillimeter Array archival data of the 1.3 mm continuum, 12 CO (2-1) and …

We present an extensive astrometric study of the protostellar binary system L 1551 IRS 5,
utilizing nearly four decades of interferometric observations obtained between 1983 and …