業績
Results
国際論文
How planetary growth outperforms migration
Temperature Structure in the Inner Regions of Protoplanetary Disks: Inefficient Accretion Heating Controlled by Nonideal
First measurements of Jupiter’s zonal winds with visible imaging spectroscopy
Gas flow around a planet embedded in a protoplanetary disc. Dependence on planetary mass
Millimeter-wave Polarization Due to Grain Alignment by the Gas Flow in Protoplanetary Disks
Water delivery by pebble accretion to rocky planets in habitable zones in evolving disks
Tensile Strength of Porous Dust Aggregates
Dependence of Hall coefficient on grain size and cosmic ray rate and implication for circumstellar disc formation
