Radio active galactic nuclei in galaxy clusters: feedback, merger signatures, and cluster tracers
Galaxy clusters, the largest gravitationally-bound structures in the universe, are composed of 50-1000s of galaxies, hot X-ray emitting gas, and dark matter. They grow in size over time through cluster and group mergers. The merger history of a cluster can be imprinted on the hot gas, known as the...
| Main Author: | |
|---|---|
| Language: | en_US |
| Published: |
2016
|
| Subjects: | |
| Online Access: | https://hdl.handle.net/2144/14065 |