Meeting Summary: Cluster Cooling Flows Become Modest


The XMM-Newton observations showing that clusters lack the emission lines predicted from massive cooling flows forced a major revision to the model, although the successor is not yet obvious. One possibility that preserves much of the original model is that the cooling gas mixes with colder gas, spending little time in the 0.2-1 keV range, but passing… (More)


3 Figures and Tables

Cite this paper

@inproceedings{SokerMeetingSC, title={Meeting Summary: Cluster Cooling Flows Become Modest}, author={Noam Soker and Joel N. Bregman} }