Origin of the high v_los feature in the Galactic bar
We analyse a controlled N-body + smoothed particle hydrodynamics simulation of a growing disc galaxy within a non-growing, live dark halo. The disc is continuously fed with gas and star particles on near-circular orbits and develops a bar comparable in size to the one of the Milky Way (MW). We extra...
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| Aineistotyyppi: | Journal article |
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Oxford University Press
2015
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