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Publication > Research Gallery > Coordinated Hydrodynamic and Astrophysical Research, Modeling, and Synthesis

Research Gallery

Coordinated Hydrodynamic and Astrophysical Research, Modeling, and Synthesis (CHARMS)

Visualization of RT Simulation Visualization of RT Simulation
nested refinement for the simulation ...(more)
Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution
Distribution of the logarithm of the mass density ρ and velocity field (unit vectors) on the equatorial plane, for Models I (left panel, non-rotating) and J (right, rotating) that include ...(more)
Two-Temperature Model for Magnetized Protostellar Outflows Two-Temperature Model for Magnetized Protostellar Outflows
Effects of temperature and magnetization on molecular outflows: the structure of the base of outflows at 1000 yr is shown with different physical conditions. Panels (a) to (c) shows the ...(more)
Disk Formation Enabled by the Hall Effect Disk Formation Enabled by the Hall Effect
Snapshots of rotationally supported disks formed by introduced Hall effect in the MHD calculations, at a representative time of 2 x 1012 sec.
Left: the edge-on view of the case ...(more)
Disk Formation Enabled by Enhanced Resistivity Disk Formation Enabled by Enhanced Resistivity
Snapshots of 2D density distributions of models with different mangetization, at a representative time of 1012 sec. The white solid lines indicate positions of the radial infall sonic transition at ...(more)
RW Aur A from the X-Wind Point of View: General Features RW Aur A from the X-Wind Point of View: General Features
Left: position-velocity diagrams of RW Aur A redshifted and blueshifted jets in [S II] emission line are shown in the upper two panels. Observed (black) and synthetic (red and blue ...(more)
Evidence of a Binary Induced Spiral From an Incomplete Ring Pattern of CIT 6 Evidence of a Binary Induced Spiral From an Incomplete Ring Pattern of CIT 6
Left: Velocity channel images of the HC3N(4–3) line emission of CIT 6 observed with the VLA (red) and modeled by a hydrodynamic radiative transfer simulation using the FLASH and SPARX ...(more)
Effects of Magnetic Field and Far-ultraviolet Radiation on the Structures of Bright-rimmed Clouds Effects of Magnetic Field and Far-ultraviolet Radiation on the Structures of Bright-rimmed Clouds
Simulated results of the bright-rimmed clouds under the influence of FUV irradiation with or without the presence of magnetic field. Physical properties shown are volumetric density, column density, temperature, magnetic ...(more)
Disk Formation through Pseudodisk Warping and Reconnections in Turbulent Magnetized Cores Disk Formation through Pseudodisk Warping and Reconnections in Turbulent Magnetized Cores
The structure of the warping pseudodisk and rotationally supported disk: close-in view of the turbulent model with persistent disk structure. The pseudodisk roughly corresponds to the red surfaces of ρ ...(more)
Disk Formation Enabled by Misalignment between Magnetic Fields and Rotation Axis Disk Formation Enabled by Misalignment between Magnetic Fields and Rotation Axis
Snapshots of 2D density distributions of models A to I. From top to bottom, the angle of magnetic field and rotational axis changes from aligned to totally misaligned. From left ...(more)
A hydrochemical hybrid code (KM2) and its benchmarks for a Photon-Dominated Region (PDR) A hydrochemical hybrid code (KM2) and its benchmarks for a Photon-Dominated Region (PDR)
Chemical abundances at the time t = 1 Myr (top) and t = 3 Myr (bottom) as a function of z-coordinates (left) and of visual extinction (right) in our hydrochemical ...(more)
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