90 citations · 448 across the 38 of their papers we have counts for
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Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres
E. Pacetti, D. Turrini, E. Schisano +13
Giant planets form in protoplanetary discs, where the coupled dynamical and chemical evolution of gas and solids determines the composition of the material they accrete. We investi…
Planet formation in chemically diverse and evolving discs -- I. Composition of planetary building blocks
E. Pacetti, E. Schisano, D. Turrini +12
Protoplanetary discs are dynamic environments where the interplay between chemical processes and mass transport shapes the composition of gas and dust available for planet formatio…
Planetesimal formation via the streaming instability in simulations of infall dominated young disks
L. -A. Hühn, C. P. Dullemond, U. Lebreuilly +7
Protoplanetary disks naturally emerge during protostellar core-collapse. In their early evolutionary stages, infalling material dominates their dynamical evolution. In the context…
The evolution of the and correlations traces protoplanetary disc dispersal
Alice Somigliana, Leonardo Testi, Giovanni Rosotti +9
(Abridged) Observational surveys of entire star-forming regions have provided evidence of power-law correlations between the disc properties and the stellar mass, especially the di…
Accuracy of ALMA estimates of young disk radii and masses. Predicted observations from numerical simulations
Ngo-Duy Tung, Leonardo Testi, Ugo Lebreuilly +7
Protoplanetary disks, which are the natural consequence of the gravitational collapse of the dense molecular cloud cores, host the formation of the known planetary systems in our u…
Protostellar chimney flues: are jets and outflows lifting submillimetre dust grains from discs into envelopes?
L. Cacciapuoti, L. Testi, L. Podio +7
Low dust opacity spectral indices () measured in the inner envelopes of class 0/I young stellar objects (age yr) have been interpreted as the presence of (sub…