Revisiting the Galactic Winds in M82. II. Development of Multiphase Outflows in Simulations
We performed a suit of three-dimensional hydrodynamical simulations with a resolution of ~10 pc to investigate the development of multiphase galactic wind in M82. The star formation and related feedback processes are solved self-consistently using a sink particle method, rather than relying on vario...
שמור ב:
| Principais autores: | , , , |
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| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
IOP Publishing
2025-01-01
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| סדרה: | The Astrophysical Journal |
| נושאים: | |
| גישה מקוונת: | https://doi.org/10.3847/1538-4357/ada38c |
| תגים: |
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