56 citations · 110 across the 10 of their papers we have counts for
10 papers
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…
The Influence of the Fractal Dimension on Dust Evolution in Protoplanetary Disks
J. E. Schöll, C. P. Dullemond, C. Dominik
Context: During the first stages of dust coagulation in protoplanetary disks, the dust aggregates are expected to have a high degree of porosity. Most models of dust growth, howeve…
Spiral formation caused by late infall onto protoplanetary disks
L. -A. Hühn, C. N. Kimmig, C. P. Dullemond
The classical picture that planet formation occurs in protoplanetary disks that are isolated from their environment is undergoing a major shift toward a more connected picture. An…
Warps survive beyond fly-by encounters in protoplanetary disks. RW Aur A as a case study
C. N. Kimmig, P. Weber, G. P. Rosotti +2
Stellar fly-bys can have multiple dynamical effects on protoplanetary disks, including warping and the excitation of spiral arms. Since observations indicate that warps are common,…
Emergence of streamers in simulations of late infall
L. -A. Hühn, C. P. Dullemond
Growing observational evidence suggests that Class II protoplanetary disks may undergo substantial interactions with their environment in the form of late infall. This mass inflow…
Late accretion offers pathway to misaligned disk around the planet-hosting IRAS 04125+2902
L. -A. Hühn, H. -C. Jiang, C. P. Dullemond
We present a 3D hydrodynamical simulation of the accretion of a gas cloudlet onto the IRAS 04125+2902 binary system, where the 3-Myr primary hosts a transiting planet. We demonstra…
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…
Formation and evolution of a protoplanetary disk: combining observations, simulations and cosmochemical constraints
Alessandro Morbidelli, Yves Marrocchi, Adnan Ali Ahmad +12
We present a plausible and coherent view of the evolution of the protosolar disk that is consistent with the cosmochemical constraints and compatible with observations of other pro…
VLT/MUSE detection of accretion-ejection associated with the close stellar companion in the HT Lup system
Sebastián Jorquera, Mickaël Bonnefoy, Laura M. Pérez +14
The accretion/ejection processes in T-Tauri stars are fundamental to their physical evolution, while also impacting the properties and evolution of the circumstellar material at a…
Rapid Formation of Massive Planetary Cores in a Pressure Bump
Tommy Chi Ho Lau, Joanna Drążkowska, Sebastian M. Stammler +2
Models of planetary core growth by either planetesimal or pebble accretion are traditionally disconnected from the models of dust evolution and formation of the first gravitational…