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What fraction of the density fluctuations in the Perseus cluster core is due to gas sloshing rather than AGN feedback? (2018)

First Author: Walker S

Attributed to: Astronomy Observation and Theory Consolidated Grant 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/sty2390

Publication URI: http://dx.doi.org/10.1093/mnras/sty2390

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2