Transition from Small-scale to Large-scale Dynamo in a Supernova-driven, Multiphase Medium

Transition from Small-scale to Large-scale Dynamo in a Supernova-driven, Multiphase Medium

Magnetic fields are now widely recognized as critical at many scales to galactic dynamics and structure, including multiphase pressure balance, dust processing, and star formation. Using imposed magnetic fields cannot reliably model the interstellar medium's (ISM) dynamical structure nor phase...

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Bibliographic Details
Main Authors: Frederick A. Gent, Mordecai-Mark Mac Low, Maarit J. Korpi-Lagg
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Astroinformatics
Astrophysical fluid dynamics
Interstellar magnetic fields
Magnetohydrodynamical simulations
Supernova dynamics
Disk galaxies
Online Access:https://doi.org/10.3847/1538-4357/ad0da0

Internet

https://doi.org/10.3847/1538-4357/ad0da0

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