RADIAL PROFILE of the 3.5 keV LINE OUT to R 200 in the PERSEUS CLUSTER

Astrophysical Journal

Volumn 829, Issue 2, 2016, Pages

  Franse, Jeroen ^a,b   Bulbul, Esra ^c   Foster, Adam ^d   Boyarsky, Alexey ^b   Markevitch, Maxim ^e   Bautz, Mark ^c   Iakubovskyi, Dmytro ^f,g   Loewenstein, Mike ^h,i   McDonald, Michael ^c   Miller, Eric ^c   Randall, Scott W ^d   Ruchayskiy, Oleg ^f   Smith, Randall K ^d  

^a LEIDEN UNIVERSITY   (Netherlands)

^b UNIVERSITEIT LEIDEN   (Netherlands)

^c MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f UNIVERSITY OF COPENHAGEN   (Denmark)

^g BOGOLYUBOV INSTITUTE FOR THEORETICAL PHYSICS   (Ukraine)

^h NASA HEADQUARTERS   (United States)

ⁱ Bldg 142   (United States)

Author keywords

dark matter; elementary particles; galaxies: clusters: individual (Perseus Cluster); line: identification; X rays: galaxies: clusters

Indexed keywords

EID: 84990941249     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.3847/0004-637X/829/2/124     Document Type: Article

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