Planets are born from the gas and dust discs surrounding young stars. Energetic radiation
from the central star can drive thermal outflows from the discs atmospheres, strongly …

We present the first volume-limited sample of cataclysmic variables (CVs), selected using
the accurate parallaxes provided by the second data release (DR2) of the European Space …

Photoevaporation of planet-forming discs by high-energy radiation from the central star is
potentially a crucial mechanism for disc evolution and it may play an important role in the …

We present a synergic study of protoplanetary disks to investigate links between inner-disk
gas molecules and the large-scale migration of solid pebbles. The sample includes 63 disks …

Young solar-type stars are known to be strong X-ray emitters and their X-ray spectra have
been widely studied. X-rays from the central star may play a crucial role in the …

Sulfur-bearing molecules play an important role in prebiotic chemistry and planet
habitability. They are also proposed probes of chemical ages, elemental C/O ratio, and grain …

Magnetized winds may be important in dispersing protoplanetary disks and influencing
planet formation. We carry out global magnetohydrodynamic simulations in axisymmetry …

We present an overview and first results from a M-band spectroscopic survey of planet-
forming disks performed with iSHELL on the Infrared Telescope Facility, using two slits that …

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 …

We present an ACA search for [C i] 1–0 emission at 492 GHz toward large T Tauri disks (gas
radii≳ 200 au) in the∼ 1–3 Myr-old Lupus star-forming region. Combined with Atacama …