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天文物理理論與觀測整合研究計畫(CHARMS)

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	Dust Radiative Transfer on a Global Hydrodynamic Simulation of a Forming Circumplanetary Disk Left – Surface density distribution of a forming circumplanetary disk in a protoplanetary disk with the Antares three-dimensional global simulation. A planet of one-Jupiter mass is placed at (x,y) = ...(more)
	Polarization Calculation and Visualization from MHD Simulation Data A sample picture based on the radiative transfer code Perspective exploring a very early stage disk formed within the MHD model of Li et al. (2014). The picture shows gas ...(more)
	Ejection History of Protostellar Outflow IRAS 04166+2706 Illustration of wind model (left) and attempts to reproduce the velocity pattern of the blue lobe of the I04166 jet (right). The upper part of the left illustration shows two ...(more)
	A Two-temperature Model of Magnetized Protostellar Outflows Density plots in log scale from simulations of two-temperature outflow model. (Left) Mosaic of simulations demonstrating effects of varying temperature and magnetization degree. Panel indices of (a) to (c) shows ...(more)
	Visualization of RT Simulation nested refinement for the simulation ...(more)
	HIGH-RESOLUTION CO OBSERVATION OF THE CARBON STAR CIT 6 Radial profiles of the 12CO J = 2–1 (left panel) and 13CO J = 2–1 (right panel) emission of the carbon star CIT6 at its systemic velocity observed by the ...(more)
	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)
	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)
	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)
	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 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 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)
	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)
	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)
	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 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)