Delivery of Dust Particles from Protoplanetary Disks onto Circumplanetary Disks of Giant Planets
N Maeda, K Ohtsuki, R Suetsugu… - The Astrophysical …, 2024 - iopscience.iop.org
The principal regular satellites of gas giants are thought to be formed by the accumulation of
solid materials in circumplanetary disks (CPDs). While there has been significant progress in …
solid materials in circumplanetary disks (CPDs). While there has been significant progress in …
Fate of a remnant solid disk around an eccentric giant planet
Context. The composition of giant planets' atmospheres is an important tracer of their
formation history. While many theoretical studies investigate the heavy-element accretion …
formation history. While many theoretical studies investigate the heavy-element accretion …
Planetesimal and planet formation in transient dust traps
Context. The ring-like structures in protoplanetary discs that are observed in the cold dust
emission by ALMA might be explained by dust aggregates trapped aerodynamically in …
emission by ALMA might be explained by dust aggregates trapped aerodynamically in …