Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence
2015; EDP Sciences; Volume: 575; Linguagem: Inglês
10.1051/0004-6361/201425278
ISSN1432-0746
AutoresC. Pinto, J. S. Sanders, Norbert Werner, J. de Plaa, A. C. Fabian, Yuying Zhang, J. S. Kaastra, A. Finoguenov, Jussi Ahoranta,
Tópico(s)Stellar, planetary, and galactic studies
ResumoContext. Feedback from active galactic nuclei, galactic mergers, and sloshing are thought to give rise to turbulence, which may prevent cooling in clusters.
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