Testing Global ISM Models: A Detailed Comparison of O VI Column Densities with FUSE and Copernicus Data
We study the O vi distribution in space and time in a representative section of the Galactic disk using three-dimensional adaptive mesh refinement hydrodynamic and magnetohydrodynamic simulations of the interstellar medium (ISM), including the disk-halo-disk circulation. The simulations describe a s...
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| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2012
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| Texto completo: | http://hdl.handle.net/10174/5605 |
| País: | Portugal |
| Oai: | oai:dspace.uevora.pt:10174/5605 |