Gaseous haloes: Linking galaxies to the IGM
In recent years, evidence has accumulated that nearby spiral galaxies are surrounded by massive haloes of neutral and ionised gas. These gaseous haloes rotate more slowly than the disks and show inflow motions. They are clearly analogous to the High Velocity Clouds of the Milky Way. We show that the...
| Main Authors: | , , , |
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| Format: | Conference item |
| Published: |
2007
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