MAPPING THE GAS TURBULENCE IN THE COMA CLUSTER: PREDICTIONS FOR ASTRO-H
Astro-H will be able for the first time to map gas velocities and detect turbulence in galaxy clusters. One of the best targets for turbulence studies is the Coma cluster, due to its proximity, absence of a cool core, and lack of a central active galactic nucleus. To determine what constraints Astro...
Main Authors: | Markevitch, M., Zhuravleva, I., ZuHone, John A. |
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Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2017
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Online Access: | http://hdl.handle.net/1721.1/108344 https://orcid.org/0000-0002-0883-9383 |
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