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 (Author), Foster, Adam (Author), Boyarsky, Alexey (Author), Markevitch, Maxim (Author), Iakubovskyi, Dmytro (Author), Loewenstein, Mike (Author), Miller, Eric (Author), Randall, Scott W. (Author), Ruchayskiy, Oleg (Author), Smith, Randall K. (Author), Bulbul, Gul E (Contributor), Bautz, Mark (Contributor), McDonald, Michael A. (Contributor), Miller, Eric D (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-04-11T13:55:33Z.
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