The formation of protostars and their disks has been understood as the result of the
gravitational collapse phase of an accumulation of dense gas that determines the mass …

Context. The formation and evolution of protoplanetary disks remains elusive. We have
numerous astronomical observations of young stellar objects of different ages with their …

Context. Due to the high visual extinction and lack of sensitive mid-infrared (MIR)
telescopes, the origin and properties of outflows and jets from embedded Class 0 protostars …

Context. Single-dish observations suggest that the abundances of organic species in star-
forming regions of the outer Galaxy, which are characterised by sub-solar metallicities, are …

Context. The origin of the chemical diversity observed around low-mass protostars probably
resides in the earliest history of these systems. Aims. We aim to investigate the impact of …

Using the MIRI medium-resolution spectrometer on JWST, we have detected pure rotational,
suprathermal OH emissions from the vicinity of the intermediate-mass protostar HOPS 370 …

Context. Signposts of early planet formation are ubiquitous in substructured young discs.
Dense, hot, and high-pressure regions that formed during the gravitational collapse process …

We use the James Webb Space Telescope (JWST) and its Mid-Infrared Instrument (MIRI)(5-
28 um), to study the embedded HH 211 flow. We map a 0.95'x0. 22'region, covering the full …

Over the past decade, progress in observational capabilities, combined with theoretical
advancements, have transformed our comprehension of the physics and chemistry during …

In this contribution, we aim to summarise the efforts of the Italian SKA scientific community in
conducting surveys of star-forming regions within our Galaxy, in the development of …