Inferring the dark matter velocity anisotropy to the cluster edge
Dark matter (DM) dominates the properties of large cosmological structures such as galaxy clusters, and the mass profiles of the DMhave been inferred for these equilibrated structures for years by using cluster X-ray surface brightnesses and temperatures. A new method has been proposed, which should...
Main Authors: | , , , , |
---|---|
Format: | Journal article |
Language: | English |
Published: |
Oxford University Press
2020
|