Turbulent dissipation in the interstellar medium: implications for galaxy formation and evolution
We study turbulent dissipation in the ISM and explore some implications forgalaxy formation and evolution using 2D MHD numerical simulations of compress-ible uids. The turbulent kinetic energy Ek is injected by stellar sources formedself-consistently in the simulation. In the ISM-like uid, regimes o...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2000
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57100913 |
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