The solid content of circumstellar disks is inherited from the interstellar medium: dust
particles of at most a micrometer in size. Protoplanetary disks are the environment where …

Protoplanetary disks are the sites of planet formation, and the evolution and eventual
dispersal of these disks strongly influences the formation of planetary systems. Disk …

We present a substantial extension of the millimeter (mm) wave continuum photometry
catalog for circumstellar dust disks in the Taurus star-forming region, based on a new" …

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 a survey at subarcsecond resolution of the 340 GHz dust continuum emission
from 50 nearby protoplanetary disks, based on new and archival observations with the …

We present a combined, homogenized analysis of archival Submillimeter Array (SMA) and
Atacama Large Millimeter/submillimeter Array (ALMA) observations of the spatially resolved …

I have used high-precision photometry and astrometry from the third data release of Gaia to
perform a survey for members of the Taurus star-forming region and young associations in …

The connection between the nature of a protoplanetary disk and that of a debris disk is not
well understood. Dust evolution, planet formation, and disk dissipation likely play a role in …

Context. Planet formation is closely related to the structure and dispersal of protoplanetary
disks. A certain class of disks, called transition disks, exhibit cavities in dust images at scales …

Aims. In the framework of the GIARPS High-resolution Observations of T Tauri stars (GHOsT)
project, we study the accretion properties of 37 classical T Tauri stars of the Taurus-Auriga …