Search for:
Search
Skip to content
Home
Intro
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: Apparent Magnetic Jet Acceleration by Strong Toroidal Magnetization
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
What’s New in CHARMS
By
Chun-Fan Liu
March 27, 2021
September 27, 2022
News Updates
IAA Quarterly Special Issue on CHARMS (2020 Summer Issue) [Chinese]
Web/Image Version
:
link
PDF Version
:
link
Bookmark the
permalink
.
«
Welcome to the CHARMS Website!
In Loving Memory of Academician Frank H. S. Shu (1943–2023)
»
error:
Content is protected !!
