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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Veröffentlicht in:	The Astrophysical journal 2024-01, Vol.961 (1), p.7
Hauptverfasser:	Gent, Frederick A., Mac Low, Mordecai-Mark, Korpi-Lagg, Maarit J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astroinformatics Astrophysical fluid dynamics Astrophysics Clustering Cosmic dust Disk galaxies Galactic structure Galaxy magnetic fields Interstellar magnetic fields Interstellar matter Interstellar medium Magnetic fields Magnetohydrodynamical simulations Modelling Multiphase Rotating generators Shear flow Star & galaxy formation Star formation Supernova Supernova dynamics Supernovae Topology
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