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Filamentary Hierarchies and Superbubbles: Galactic Multiscale Magnetohydrodynamic Simulations of Giant Molecular Cloud to Star Cluster Formation

There is now abundant observational evidence that star formation is a highly dynamical process that connects filament hierarchies and supernova feedback from galaxy-scale kiloparsec filaments and superbubbles to giant molecular clouds (GMCs) on 100 pc scales and star clusters (1 pc). Here we present...

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Bibliografiske detaljer
Principais autores: Bo Zhao, Ralph E. Pudritz, Rachel Pillsworth, Hector Robinson, James Wadsley
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2024-01-01
Serier:The Astrophysical Journal
Fag:
Online adgang:https://doi.org/10.3847/1538-4357/ad67e2
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