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The distance to the Norma cluster and its relation to the great attractor region
The Local Group's peculiar motion with respect to the cosmic microwave background has been measured with high precision and found to be ~627±22 km s-1, but the source of this motion is not clear. Studies to constrain the fractional contribution of the local mass overdensity, particularly in the Grea...
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| Language: | English |
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Department of Astronomy
2015
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