Searching for Extreme-BCG Clusters at 0.2 < z < 1.3
Active galactic nuclei (AGN) feedback is believed to be responsible for counteracting the formation of the classical “cooling flow”, predicted to be associated with most “cool core” clusters of galaxies. Several studies have shown that many phenomena found in galaxy clusters can be neatly explained...
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Format: | Thesis |
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Massachusetts Institute of Technology
2022
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Online Access: | https://hdl.handle.net/1721.1/142831 |