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Simulations of the dynamics of magnetized jets and cosmic rays in galaxy clusters

ABSTRACT. Feedback processes by active galactic nuclei in the centres of galaxy clusters appear to prevent large-scale cooling flows and impede star formation.

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Bibliographic Details
Main Authors: Ehlert, Kristian (Author) , Pakmor, Rüdiger (Author) , Springel, Volker (Author) , Pfrommer, Christoph (Author)
Format: Article (Journal)
Language:English
Published: 2018 September 4
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 3, Pages: 2878-2900
ISSN:1365-2966
DOI:10.1093/mnras/sty2397
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2397
Verlag, Volltext: https://academic.oup.com/mnras/article/481/3/2878/5090410
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Author Notes:K. Ehlert, R. Weinberger, C. Pfrommer, R. Pakmor and V. Springel
Description
Summary:ABSTRACT. Feedback processes by active galactic nuclei in the centres of galaxy clusters appear to prevent large-scale cooling flows and impede star formation.
Item Description:Gesehen am 23.01.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2397

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