CHARMS
 
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  • Home
  • Introduction
  • Science
    • Interstellar Medium, Clouds and Cores
    • Photo-Dominating Regions
      • Structure of Bright-Rimmed Clouds
    • Magnetized Gravitational Collapse and Formation of Earliest Disks
      • Magnetic Spirals in Accretion Flows Originated from Misaligned Magnetic Fields
      • Time Evolution of 3D Disk Formation with Misaligned Axes
      • Disk Formation in Turbulent Magnetized Cloud Cores
      • Misalignment between Magnetic Field and Rotation
      • Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution
      • Disk Formation Enabled by the Hall Effect
      • Disk Formation Enabled by Enhanced Resistivity
    • Molecular Jets and Outflows from Earliest Phases
      • A Unified Model for Bipolar Outflows from Young Stars: Kinematic Signatures of Jets, Winds, and Their Magnetic Interplay with the Ambient Toroids
      • A Unified Model for Bipolar Outflows from Young Stars: Interplay of Magnetized Wide-Angle Wind and Isothermal Toroids
      • Two-Temperature Model for Magnetized Protostellar Outflows
      • A Unified Model for Bipolar Outflows from Young Stars
    • Jets and Winds in Time
      • Ejection History of the IRAS 04166+2706 Molecular Jet
      • Molecular Jet of IRAS 04166+2706
      • RW Aur A Jet from the X-Wind Point of View
      • The [Ne III] Jet of DG Tau and its Ionization Scenarios
      • Velocity-resolved [Ne III] from X-Ray Irradiated Sz 102 Microjets
    • Formation and Evolution of Protoplanetary and Circumplanetary Disks
      • Ring and Gap Formation in Wind-Launching Disks: 3D Simulations
      • Ring and Gap Formation in Wind-Launching Disks: Ambipolar Diffusion and Reconnection
      • Ring and Gap Formation in Wind-Launching Disks: 2D Axisymmetric Simulations
      • The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps
    • Star-Disk Interactions
      • Three-Dimensional MHD Simulations of Star-Disk Interactions
      • Magnetospheric Accretion and Ejection of Matter in Resistive MHD Simulations
    • Meteoritic Connections
    • Evolved Stars and Circumstellar Envelopes
      • Binary-Induced Bifurcation in Superwind Spiral Pattern
      • Binary-Induced Spiral from AGB Star
  • Code Development
    • X-Wind Modeling
    • MHD/HD Code Development
    • Chemistry and Chemical Evolution
    • Radiative Transfer
    • GPU Code Development
  • People
  • Publications
  • Facilities
    • HPC
    • NanoSIMS
  • Workshops/Schools
    • 2018
    • 2017
    • 2016

Facilities

High-Performance Computing (HPC)

Nanoscale Secondary Ion Mass Spectrometry (NanoSIMS)

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