The Structure and Composition of Multiphase Galactic Winds in a Large Magellanic Cloud Mass Simulated Galaxy

The Structure and Composition of Multiphase Galactic Winds in a Large Magellanic Cloud Mass Simulated Galaxy

We present the first results from a high-resolution simulation with a focus on galactic wind driving for an isolated galaxy with a halo mass of ∼10 ^11 M _⊙ (similar to the Large Magellanic Cloud) and a total gas mass of ∼6 × 10 ^8 M _⊙ , resulting in ∼10 ^8 gas cells at ∼4 M _⊙ mass resolution. We...

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Bibliographic Details
Main Authors: Ulrich P. Steinwandel, Chang-Goo Kim, Greg L. Bryan, Eve C. Ostriker, Rachel S. Somerville, Drummond B. Fielding
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galactic winds
Galaxy evolution
Hydrodynamical simulations
Stellar feedback
Interstellar medium
Online Access:https://doi.org/10.3847/1538-4357/ad09e1

Internet

https://doi.org/10.3847/1538-4357/ad09e1

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