Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster

We present new, deep observations of the Phoenix cluster from Chandra, the Hubble Space Telescope, and the Karl Jansky Very Large Array. These data provide an order-of-magnitude improvement in depth and/or angular resolution over previous observations at X-ray, optical, and radio wavelengths. We fin...

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Bibliographic Details
Main Authors: McDonald, M. (Author), McNamara, B. R. (Author), Voit, G. M. (Author), Bayliss, Matthew B (Author), Benson, B. A. (Author), Brodwin, M. (Author), Canning, R. E. A. (Author), Florian, M. K. (Author), Garmire, G. P. (Author), Gaspari, M. (Author), Gladders, M. D. (Author), Hlavacek-Larrondo, J. (Author), Kara, Erin A (Author), Reichardt, C. L. (Author), Russell, H. R. (Author), Saro, A. (Author), Sharon, K. (Author), Somboonpanyakul, T. (Author), Tremblay, G. R. (Author), Weeren, R. J. van (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Astronomical Society, 2020-11-18T22:35:21Z.
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