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Stirring Up the Pot: Can Cooling Flows In Galaxy Clusters Be Quenched By Gas Sloshing?

ASTROPHYSICAL JOURNAL, no. 2 (2010): 908.0-928.0

Cited: 71|Views24

Abstract

X-ray observations of clusters of galaxies reveal the presence of edges in surface brightness and temperature, known as "cold fronts." In relaxed clusters with cool cores, these commonly observed edges have been interpreted as evidence for the "sloshing" of the core gas in the cluster's gravitational potential. Such sloshing may provide a...More

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R. E. Johnson
R. E. Johnson
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