Giant planets can interact with multiple and chemically diverse environments in
protoplanetary disks while they form and migrate to their final orbits. The way this interaction …

Context. The field of exo-atmospheric characterisation is progressing at an extraordinary
pace. Atmospheric observations are now available for tens of exoplanets, mainly hot and …

Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate
the physico-chemical properties of the atmospheres. Their inferred chemical composition is …

The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To
guarantee that the C/O ratio provides robust information, we need to accurately quantify the …

Context. Exoplanetary properties strongly depend on stellar properties: to know the planet
with accuracy and precision it is necessary to know the star as accurately and precisely as …

The disk midplane temperature is potentially affected by the dust traps/rings. The dust
depletion beyond the water snowline will cast a shadow. In this study, we adopt a detailed …

One of the main objectives of the European Space Agency's Ariel telescope (launch 2029) is
to understand the formation and evolution processes of a large sample of planets in our …

We report the first simulations of planetary system dynamics as affected by an embedded
cluster environment. Such environments are generally believed to be relevant for the large …

Context. In 2020 the European Space Agency selected Ariel as the next mission to join the
space fleet of observatories to study planets outside our Solar System. Ariel will be devoted …

Theoretical physical-chemical models for the formation of planetary systems depend on data
quality for the Sun's composition, that of stars in the solar neighbourhood, and of the …