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...
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| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2025-01-01
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| Colecção: | The Astrophysical Journal |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/1538-4357/ada38c |
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