CompAS Project Scientist
Star formation, MHD simulations
Observational signatures of early disk formation by MHD models
An early disk in formation from collapsing magnetic flows
Polarization Calculation and Visualization from MHD Simulation Data
Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution
Two-Temperature Model for Magnetized Protostellar Outflows
Disk Formation Enabled by the Hall Effect
Disk Formation Enabled by Enhanced Resistivity
Disk Formation through Pseudodisk Warping and Reconnections in Turbulent Magnetized Cores
Disk Formation Enabled by Misalignment between Magnetic Fields and Rotation Axis
A hydrochemical hybrid code (KM2) and its benchmarks for a Photon-Dominated Region (PDR)