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The Collisions of HVCs with a Magnetized Gaseous Galactic Disk
We discuss 2-D MHD numerical simulations for the interaction of high-velocit y clouds with a magnetized Galactic disk. The initial magnetic field is oriented parallel to the disk, and we consider two different field topologies: parallel and perpendicular to the plane of motion of the clouds. The imp...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Main Authors: | , , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2001
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57101122 |
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