Since Protostars and Planets VI (PPVI), our knowledge of the global properties of
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …

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 …

Dust particle sizes constrained from dust continuum and polarization observations by radio
interferometry are inconsistent by at least an order of magnitude. Motivated by porous dust …

Context. The evolution of protoplanetary disks is regulated by an interplay of several
processes, either internal to the system or related to the environment. As most of the stars …

Abstract We present Markov Chain Monte Carlo radiative transfer modeling of a joint ALMA
345 GHz and spectral energy distribution data set for a sample of 97 protostellar disks from …

Most stars, including the Sun, are born in rich stellar clusters containing massive stars.
Therefore, the study of the chemical reservoir of massive star-forming regions is crucial to …

The total number of dust grains in protoplanetary disks is one of the key properties that
characterizes the potential for planet formation. With (sub-) millimeter flux measurements …

Context. Surveys of protoplanetary disks in nearby star-forming regions (SFRs) have
provided important information on their demographics. However, due to their sample sizes …

Context. Observations of interstellar material infalling onto star-and planet-forming systems
have become increasingly common thanks to recent advancements in radio interferometry …

Context. Many population studies have been performed over the past decade with the
Atacama Large millimeter/submillimeter Array (ALMA) to understand the bulk properties of …