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...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Ngā kaituhi matua: | , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2000
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57100913 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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