RADIAL PROFILE OF THE 3.5 keV LINE OUT TO R[subscript 200] IN THE PERSEUS CLUSTER

RADIAL PROFILE OF THE 3.5 keV LINE OUT TO R[subscript 200] IN THE PERSEUS CLUSTER

The recent discovery of the unidentified emission line at 3.5 keV in galaxies and clusters has attracted great interest from the community. As the origin of the line remains uncertain, we study the surface brightness distribution of the line in the Perseus cluster since that information can be used...

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Bibliographic Details
Main Authors: Franse, Jeroen, Foster, Adam, Boyarsky, Alexey, Markevitch, Maxim, Iakubovskyi, Dmytro, Loewenstein, Mike, Miller, Eric, Randall, Scott W., Ruchayskiy, Oleg, Smith, Randall K., Bulbul, Gul E, Bautz, Mark, McDonald, Michael A., Miller, Eric D
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/108040
https://orcid.org/0000-0001-5226-8349

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