The disks that orbit young stars are the essential conduits and reservoirs of material for star
and planet formation. Their structures, meaning the spatial variations of the disk physical …

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 …

The disk mass is among the most important input parameter for every planet formation
model to determine the number and masses of the planets that can form. We present an …

Aims. We aim to study vertical settling and radial drift of dust in protoplanetary disks from a
different perspective: an edge-on view. An estimation of the amplitude of settling and drift is …

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 …

Gaps in protoplanetary disks have long been hailed as signposts of planet formation.
However, a direct link between exoplanets and disks remains hard to identify. We present a …

Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …

We present ALMA observations of 106 G-, K-, and M-type stars in the Upper Scorpius OB
Association hosting circumstellar disks. With these data, we measure the 0.88 mm …

The mass of a protoplanetary disk limits the formation and future growth of any planet.
Masses of protoplanetary disks are usually calculated from measurements of the dust …

Context. The formation of planets strongly depends on the total amount as well as on the
spatial distribution of solids in protoplanetary disks. Thanks to the improvements in …