Spiral galaxy HI models, rotation curves and kinematic classifications
Although galaxy interactions cause dramatic changes, galaxies also continue to form stars and evolve when they are isolated. The dark matter (DM) halo may influence this evolution since it generates the rotational behaviour of galactic disks which could affect local conditions in the gas. Therefore...
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| Language: | en_US |
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2011
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| Online Access: | http://hdl.handle.net/1993/4377 |
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