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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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發表在:Revista Mexicana de Astronomía y Astrofísica
Main Authors: Alfredo Santillán, Marco Martos, José Franco, Jongsoo Kim
格式: Artigo
語言:Inglês
出版: Universidad Nacional Autónoma de México 2001
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在線閱讀:https://www.redalyc.org/articulo.oa?id=57101122
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