Exploring the Formation of Resistive Pseudodisks with the GPU Code Astaroth
Pseudodisks are dense structures formed perpendicular to the direction of the magnetic field during the gravitational collapse of a molecular cloud core. Numerical simulations of the formation of pseudodisks are usually computationally expensive with conventional CPU codes. To demonstrate the proof...
Main Authors: | Miikka S. Väisälä, Hsien Shang, Daniele Galli, Susana Lizano, Ruben Krasnopolsky |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acfb00 |
Similar Items
-
Outflows Driven from a Magnetic Pseudodisk
by: Shantanu Basu, et al.
Published: (2024-01-01) -
A Unified Model for Bipolar Outflows from Young Stars: Apparent Magnetic Jet Acceleration
by: Hsien Shang, et al.
Published: (2023-01-01) -
The Formation of Star-forming Disks in the TNG50 Simulation
by: Enci Wang, et al.
Published: (2023-01-01) -
Angular Momentum Transport in Binary Star Formation: The Enhancement of Magnetorotational Instability and Role of Outflows
by: Tomoaki Matsumoto
Published: (2024-01-01) -
Coevolution of Stars and Gas: Using an Analysis of Synthetic Observations to Investigate the Star–Gas Correlation in STARFORGE
by: Samuel Millstone, et al.
Published: (2023-01-01)