The Xmm Cluster Survey: New Evidence for the 3.5-Kev Feature in Clusters Is Inconsistent with a Dark Matter Origin

AuthID
 P-00S-V7T
17
Author(s)
Bhargava, S
·
Giles, PA
·
Romer, AK
·
Jeltema, T
·
Bermeo, A
·
Hilton, M
·
Wilkinson, R
·
Vergara, C
·
Collins, CA
·
Manolopoulou, M
·
Rosborough, S
·
Stott, JP
·
Swann, E
·
Document Type
Article
Year published
2020
Published
in MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN: 0035-8711
Volume: 497, Issue: 1, Pages: 656-671 (16)
Indexing
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Scopus®
Crossref®14
Google Scholar®
Publication Identifiers
SCOPUS: 2-s2.0-85096615234
Wos: WOS:000574919600047
Source Identifiers
ISSN: 0035-8711
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