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 …

The strong X-ray irradiation from young solar-type stars may play a crucial role in the
thermodynamics and chemistry of circumstellar discs, driving their evolution in the last …

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 …

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 …

Theoretical models indicate that photoevaporative and magnetothermal winds play a crucial
role in the evolution and dispersal of protoplanetary disks and affect the formation of …

The evolution of young stars and disks is driven by the interplay of several processes,
notably the accretion and ejection of material. These processes, critical to correctly describe …

We analyze high-resolution (Δv≤ 10 km s− 1) optical and infrared spectra covering the [O i]
λ6300 and [Ne ii] 12.81 μm lines from a sample of 31 disks in different evolutionary stages …

PDS 70 is so far the only young disk where multiple planets have been detected by direct
imaging. The disk has a large cavity when seen at submillimeter and near-infrared …

Magnetohydrodynamic (MHD) and photoevaporative winds are thought to play an important
role in the evolution and dispersal of planet-forming disks. Here, we analyze high-resolution …